Preprints in 2019
PP 019107
Physics of Eclipsing Binaries. IV. The impact of interstellar extinction on the light curves of eclipsing binaries
(1) IAC, (2) ULL, (3) Villanova, (4) Ljubjana, (5) Eastern, (6) AAVSO, (7) Sheffield, (8) NCAC
PP 019106
Metallicity and α-element Abundance Gradients along the Sagittarius Stream as Seen by APOGEE
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019105
Ionization correction factors for sodium, potassium, and calcium in planetary nebulae
(1) IA-UNAM, Mexico, (2) IAC, Spain, (3) ULL, Spain
PP 019104
Triaxiality can explain the alleged dark matter deficiency in some dwarf galaxies
(1) Instituto de Astrof ́ısica de Canarias, La Laguna, Spain,
(2) Universidad de La Laguna,
(3) Faculty of Engineering, University Oporto, Oporto, Portugal,
(4) CENTRA/SIM, Faculty of Sciences, University Lisbon, Lisbon, Portugal
PP 019103
Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019102
USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius
(1) IAC, (2) ULL, (3) Universidad de Chile, (4) University of Zielona Go ́ra, Poland, (5) Centro de Astrobiología, (6) CSIC, (7) Universidad Politécnica de Cartagena, (8) W. M. Keck Observatory, USA.
PP 019101
First Evidence of Enhanced Recombination in Astrophysical Environments and the Implications for Plasma Diagnostics
(1) Auburn University, USA, (2) Princeton University , USA, (3) University of West Georgia, USA, (4) CfA, Harvard, USA, (5) IAC, Spain, (6) ULL, Spain, (7) Rice University, USA, (8) Queen's University Belfast, UK
PP 019100
El campo de túmulos de Peñas Pasera de la ciudad celtibérica de Aratis (Arande del Moncayo, Zaragoza) y el calendario celta
(1) IAC, (2) Dirección General de Cultura y Patrimonio del Gobierno de Aragón
PP 019099
Kinematic and metallicity properties od the Aquarius dwarf galaxy from FORS2 MXU spectroscopy
1 Instituto de Astrofísica de Andalucía - CSIC, Glorieta de la Astronomía s/n, 18008 Granada, Spain
2 Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
3 Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain
4 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
5 European Southern Observatory, Karl-Schwarzschild Strasse 2, D-85748 Garching, Germany
6 Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany
7 School of Natural Sciences, University of Tasmania, Private Bag 37 Hobart, Tasmania 7001, Australia
8 Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), 1290 Sauverny,
Switzerland
9 GEPI, CNRS UMR 8111, Observatoire de Paris, PSL Research University, F-92125, Meudon, Cedex, France
10 National Research Council, Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, BC V9E 2E7,
Canada
11 Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
12 Kapteyn Astronomical Institute, University of Groningen, 9700AV Groningen, The Netherlands
PP 019098
Planetary Nebulae seen by TESS: Results and discovery of new binary central star candidates from Cycle 1
(1) CAB, (2) SVO), (3) IAC, (4) ULL, (5) IAA
PP 019097
A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph
MPIA, Heidelberg, Germany; Department of Astrophysics; University Vienna, Wien, Austria; Instituto de Astrofisica de Canarias, Tenerife, Spain; Departamento de Astrofisica, Universidad de La Laguna, enerife, Spain
PP 019096
Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. II. Second year of LP15 observations
(1) Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
(2) Universidad de La Laguna, Departamento de Astrofísica, 38206 La Laguna, Tenerife, Spain
(3) University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban 4000, South Africa
(4) Tartu Observatory, University of Tartu, Observatooriumi 1, 61602 Tõravere, Estonia
PP 019095
The Vanishing & Appearing Sources during a Century of Observations project: I. USNO objects missing in modern sky surveys and follow-up observations of a "missing star"
(1) Nordita, Stockholm, Sweden; (2) IAC; (3) Department of Information Technology, Uppsala University, Sweden; (4) University of Oulu, Astronomy Research Unit, Finland; (5) ULL; and other centers.
PP 019094
Carbon, nitrogen and oxygen abundance gradients in M101 and M31
(1) IAC, (2) Departamento de Astrofísica, ULL, (3) Institute for Astronomy (University of Hawaii)
PP 019093
Simultaneous longitudinal and transverse oscillations in filament threads after a failed eruption
(1) Center of Excellence in Space Sciences India, Indian Institute of Science Education and Research Kolkata, West Bengal, India
(2) Indian Institute of Astrophysics, Bangalore, India
(3) Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Leuven, Belgium
(4) Instituto de Astrofísica de Canarias
(5) Universidad de La Laguna
PP 019092
NGC 6240: A triple nucleus system in the advanced/final state of merging
(1) Institut für Astrophysik, Universität Göttingen, (2) Leibniz-Institut für Astrophysik Potsdam (AIP), (3) Physics Department and the Haifa Research Center for Theoretical Physics and Astrophysics, University of Haifa, (4) Instituto de Astrofísica de Canarias (IAC), (5) Universidad de La Laguna, (6) Univ Lyon, Univ Lyon1, Ens de Lyon, (7) Institut de Recherche en Astrophysique et Planétologie (IRAP)
PP 019090
Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. II. 3D asymmetrical kinematics of mono-age populations in the disk between 6−14 kpc
(1) South−Western Institute for Astronomy Research, Yunnan University,
Kunming, 650500, P. R. China; (2) Department of Astronomy, China West Normal University, Nanchong 637009, China; (3) IAC; (4) ULL; y otros.
PP 019089
Life in the fast lane: a direct view of the dynamics, formation, and evolution of the Milky Way's bar
Several institutions from Canada and South America and Europe (including IAC and ULL)
PP 019088
Uncovering the birth of the Milky Way through accurate stellar ages with Gaia.
(1): Instituto de Astrofísica de Canarias, La Laguna, Spain; (2): Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Spain; (3): Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Nice, France; (4): INAF – Astronomical Observatory of Abruzzo, Teramo, Italy
PP 019087
The Hubble Catalog of Variables (HCV)
(1) National Observatory of Athens,
(2) Department of Physics and Astronomy, Michigan State University,
(3) Sternberg Astronomical Institute, Moscow State University
(4) RHEA Group for ESA-ESAC
(5) Department of Physics, National and Kapodistrian University of Athens
(6) Athena Research and Innovation Center
(7) Instituto de Astrofísica de Canarias
(8) ESA, European Space Astronomy Centre
(9) Space Telescope Science Institute
(10) Quasar Science Resources for ESA-ESAC
(11) The Johns Hopkins University
(12) Institute of Astrophysics, FORTH, Heraklion
(13) Department of Physics, Univ. of Crete
(14) American Community Schools of Athens,
(15) Greek Research and Technology Network, Athens
(16) INAF-Osservatorio Astronomico di Capodimonte
PP 019086
Coronal cooling as a result of mixing by the nonlinear Kelvin-Helmholtz instability
(1) CEMPS University of Exeter
(2) Instituto de Astrofisica de Canarias
(3) Universidad de La Laguna
PP 019084
Physical parameters of the torus for the type 2 Seyfert IC 5063 from mid-IR and X-ray simultaneous spectral fitting
(1) IRyA, (2) UNAM, (3) IAC, (4) ULL
PP 019083
Enduring Sacred Places: The Astronomical Orientation of the Iberian Cave-Sanctuary of Cueva Santa del Cabriel in Spain
(1) University of Valencia, (2) IAC, (3) Independent Scholar
PP 019082
ALMA images the many faces of the NGC1068 torus and its surroundings
(1) OAN; (2) Observatoire de Paris; (3) IAC; (4) ULL
PP 019081
Exploring the mid-infrared SEDs of six AGN dusty torus models II: the data
(1) IRyA; (2) IAA; (3) University of Oxford; (4) IAC; (5) ULL
PP 019080
Exploring the mid-infrared SEDs of six AGN dusty torus models I: synthetic spectra
(1) IRyA; (2) IAA; (3) University of Oxford; (4) IAC; (5) ULL
PP 019079
Title:Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017
1-INAF - Istituto di Radioastronomia, Bologna, Italy; 2-INAF - Osservatorio Astrofisico di Torino, Torino, Italy;
3- Instituto de Astrofisica de Canarias (IAC), Spain; 4-Dpto. Astrofisica, ULL, Spain; 5- Instituto de Astrofísica de Andalucía, Spain; 6- Pulkovo Observatory, Russia; 7- Institute of Astronomy and NAO, Bulgaria; 8- Crimean Astrophysical Observatory, Russia
PP 019078
Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. Part III: A new velocity substructure and time stamps of the Galactic disk asymmetry in the disk between 12−15 kpc
(1) South−Western Institute for Astronomy Research, Yunnan University, Kunming, 650500, P. R. China; (2) Department of Astronomy, China West Normal University, Nanchong 637009, China; (3) LSST, 950 North Cherry Avenue, Tucson, AZ 85719, USA; 4) IAC; (5) ULL
PP 019077
Fullerenes in the IC 348 star cluster of the Perseus Molecular Cloud
Instituto de Astrofísica de Canarias
UNiversidad de La Laguna
PP 019076
The beamed jet and quasar core of the distant blazar 4C 71.07
(1) Osservatorio Astrofisico di Torino - Italy, (2) IAC - Spain, (3) Departamento de Astrofisica, ULL - Spain, (4) Ulugh Beg Astronomical Institute, Maidanak Observatory - Uzbekistan, (5) Astronomical Institute, St. Petersburg - Russia, (6) Pulkovo Observatory, St. Petersburg - Russia, (7) Osservatorio Astronomico di Brera - Italy
PP 019075
On the triple-star origin of the planetary nebula Sh 2-71
(1) IAC, (2) ULL, (3) Charles University, (4) GTC
PP 019074
Spatial variations in the Milky Way disc metallicity-age relation
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019073
Accretion and Outflow in V404 Cyg
(1) IAC, (2) ULL, (3) Univ. of Manchester, (4)Univ. of Oxford, (5) Univ. of Southampton, (6) SRON
PP 019072
On the ultra-compact nature of the neutron star system 1RXS J170854.4-321857: insights from X-ray spectroscopy
(1) IAC, (2) ULL, (3), Universidad de Valparaíso
PP 019071
Inferring the 3-D shapes of extremely metal-poor galaxies from sets of projected shapes
((1) Instituto de Astrofisica de Canarias, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, Spain, (3) IBM Research Division, Watson Research Center, USA, (4) Department of Physics & Astronomy, Vassar College, USA)
PP 019070
Quantifying the AGN-driven outflows in ULIRGs (QUADROS) IV: HST/STIS spectroscopy of the sub-kpc warm outflow in F14394+5332
(1) University of Sheffield, (2) IAC, (3) ULL, (4) Florida Institute of Technology
PP 019069
Fundamental Transverse Vibrations of the Active Region Solar Corona
(1) IAC, (2) ULL, (3) Universitat de les Illes Balears, (4) Institute of Applied Computing & Community Code, (4) University of St Andrews
PP 019068
Do evolved stars in the LMC show dual dust chemistry?
(1)Univ. Roma Tre; (2) IAC-ULL; (3) Koninklijke Sterrenwacht van Belgi; (4) ASI-Roma; (5) OAR-INAF; (6) UAM
PP 019067
Hard-state accretion disk winds from black holes: the revealing case of MAXI J1820+070
(1) IAC, (2) ULL, (3) University of Manchester, (4) Osservatorio astronomico di Brera, (5) University of Oxford, (6) SAAO, (7) University of Notre Dame, (8) ESO, (9) University of Warwick
PP 019066
Hard-state accretion disk winds from black holes: the revealing case of MAXI J1820+070
(1) IAC, (2) ULL, (3) University of Manchester, (4) Osservatorio astronomico di Brera, (5) University of Oxford, (6) SAAO, (7) University of Notre Dame, (8) ESO, (9) University of Warwick
PP 019064
Distribution of red clump stars does not support the X-shaped Galactic bulge
(1) IAC, (2) ULL, (3) Center for Galaxy Evolution Research & Department of Astronomy, Yonsei University, Seoul 03722, Republic of Korea
PP 019063
Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
(1) IAC
(2) Dpto. de Astrofísica. Univ. de La Laguna
(3) School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban, 4000, South Africa
(4) Tartu Observatory, University of Tartu, Observatooriumi 1, 61602, Toravere, Estonia
PP 019062
Formation and morphology of anomalous solar circular polarization
IAC , Istituto Ricerche Solari Locarno
PP 019061
TOI-150: A transiting hot Jupiter in the TESS southern CVZ
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019060
The metal-rich halo component extended in z: a characterization with Gaia DR2 and APOGEE
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019058
Title:The fundamental metallicity relation emerges from the local anti-correlation between star formation rate and gas-phase metallicity existing in disk galaxies
IAC and Department of Astrophysics, ULL, Spain
PP 019057
A near-infrared study of the multi-phase outflow in the type-2 quasar J1509+0434
(1) IAC, (2) ULL, (3) University of Sheffield, (4) Institute of Astronomy, Cambridge, (4) INAF - Osservatorio Astronomico di Brera
PP 019056
Stellar content, planetary nebulae, and globular clusters of [KKS2000]04 (NGC1052-DF2)
(1) IAC (2) ULL (3) CENTRA-Ci\^{e}ncias, Science Faculty, University of Lisbon (4) University of Oporto
PP 019055
Detection limits of exoplanetary atmospheres with 2-m class telescopes
(1) AI-CAS, (2) Masaryk University, (3) ESO, (4) IAC, (5) ULL
PP 019053
Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry
[1] KULeuven, [2] IAC/ULL
PP 019052
Do AGN triggering mechanisms vary with radio power? I.Optical morphologies of radio-intermediate HERGs
(1) University of Sheffield, (2) IAC, (3) ULL, (4) Pontificia Universidad Católica de Chile
PP 019051
Discovery of an old nova remnant in the Galactic globular cluster M 22
(1) Institut für Astrophysik, Georg-August-Universität Göttingen, (2) Leibniz-Institut für Astrophysik Potsdam (AIP), (3) Astrophysics Research Institute, Liverpool John Moores University, (4) Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, (5) Leiden Observatory, Leiden University, (6) Institut für Physik und Astronomie, Universität Potsdam, (7) Instituto de Astrofísica de Canarias (IAC), (8) Universidad de La Laguna, Dpto. Astrofísica, (9) Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon
PP 019050
AGB dust and gas ejecta in extremely metal-poor environments
(1) IAC-ULL; (2) INAF-OAR; (3) Macquarie University-AAARC
PP 019049
Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
(1) IAC, (2) ULL, (3) Biruni Observatory, Shiraz University, Shiraz, Iran (4) Physics Department, Shiraz University, Shiraz, Iran (5) Faculty of Physics, Kharazmi University, Tehran, Iran
PP 019048
Normal modes of transverse coronal loop oscillations from numerical simulations: I. Method and test case
(1) Departament de Física, Universitat de les Illes Balears, 07122 Palma de Mallorca, Spain
(2) Instituto de Astrofísica de Canarias, 38205 La Laguna, Spain
(3) Departamento de Astrofísica, Universidad de La Laguna, 38206, La Laguna, Spain
(4) Institute of Applied Computing & Community Code (IAC3), UIB, Spain
PP 019047
Spectropolarimetric analysis of an active region filament. II. Evidence of the limitations of a single component model
IAC, ULL
PP 019046
Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions
IAC, ULL
PP 019045
Torus model properties of an ultra-hard X-ray selected sample of Seyfert galaxies
(1) IAC, (2) ULL
PP 019044
Polarization of changing-look quasars
(1) Université de Liège, (2) Instituut voor Sterrenkunde, (3) Université de Strasbourg, (4) IAC, (5) ULL
PP 019043
The Fornax 3D project: Thick disks in a cluster environment
(1) Instituto de Astrofísica de Canarias, (2) Depto. Astrofísica, Universidad de La Laguna, (3) Astrophysics Research Institute, Liverpool John Moores University, (4) European Southern Observatory, (5) Dipartimento di Fisica e Astronomia 'G. Galilei', Università di Padova, (6) INAF-Osservatorio Astronomico di Padova, (7) Sterrewacht Leiden, Leiden University, (8) Max-Planck-Institut fuer extraterrestrische Physik, (9) INAF-Osservatorio Astronomico di Capodimonte, (10) Max-Planck Institut fuer Astronomie, (11) University of California Observatories, (12) Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama, (13) Armagh Observatory and Planetarium, (14) Department of Astrophysics, University of Vienna, (15) Sterrenkundig Observatorium, Universiteit Gent, (16) Centre for Astrophysics Research, University of Hertfordshire, (17) Department of Physics and Astronomy, Macquarie University, (18) Australian Astronomical Observatory
PP 019042
Multiwavelength spectroscopy of the black hole candidate MAXI J1813-095 during its discovery outburst
(1) Instituto de Astrofísica de Canarias (IAC), (2) Departamento de Astrofísica, Universidad de La Laguna, (3) Nicolaus Copernicus Astronomical Center, (4) European Southern Observatory (ESO), (5) SRON
PP 019041
Title:Astro2020 Science White Paper: Stellar Physics and Galactic Archeology using Asteroseismology in the 2020's
* IAC/ULL
PP 019040
Two is a Crowd? Characterising the effect of photometric contamination on the extraction of the global asteroseismic parameter $ν_{\text{max}}$ in Red-Giant Binaries
* IAC/ULL
PP 019039
Stellar Astrophysics and Exoplanet Science with the Maunakea Spectroscopic Explorer (MSE)
* IAC/LLa
PP 019038
Mixed properties of fast MHD waves in non-uniform plasmas
(1) Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Leuven, Belgium
(2) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
(3) Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife, Spain
PP 019037
Spotting the differences between active and non-active twin galaxies on kpc-scales. A pilot study
(1) IAC, (2) ULL, (3) UNAM, (4) UAM, (5) IAA
PP 019036
Inference of magnetic field strength and density from damped transverse coronal waves
Instituto de Astrofisica de Canarias, E-38205, La Laguna, Tenerife, Spain
Departamento de Astrofisica, Universidad de La Laguna, E-38206, La Laguna, Tenerife, Spain
PP 019034
Surface abundances of CNO in Galactic O-stars: a pilot study with FASTWIND
(1) LMU München, Universitätssternwarte
(2) IAC/ULL
PP 019033
Discovery of Resolved Magnetically Split Lines in SDSS/APOGEE Spectra of 157 Ap/Bp Stars
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019032
Exploration of long-period oscillations in an H$alpha$ prominence
(1) Astronomical Institute ASCR, Fricova 298, 251 65 Ond ˇ ˇrejov, Czech Republic
(2) LESIA, Observatoire de Paris, PSL Research University, CNRS Sorbonne Université, Univ. Paris 06, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, Meudon, 92195, France
(3) SUPA School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, UK
(4) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
(5) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
PP 019031
The VLT-FLAMES Tarantula Survey XXXI. Radial velocities and multiplicity constraints of red supergiant stars in 30 Doradus
1. IAC,
2. ULL,
3. Department of Computer Science and Mathematics, European Space Astronomy Centre (ESAC), Camino bajo del Castillo s/n, Urbanizacion Villafranca del Castillo, Villanueva de la Cañada, 28 692 Madrid, Spain
4. UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK
5. Institute of astrophysics, KU Leuven, Celestijnlaan 200D, 3001, Leuven, Belgium
6. Departamento de F\'isica Te\'orica e Experimental, Universidade Federal do Rio Grande do Norte, CP 1641, Natal, RN, Brazil
7. School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK
8. Department of Physics, University of Surrey, Guildford GU2 7XH, UK
9. Institut de Ci\`{e}ncies del Cosmos (ICCUB), Universitat de Barcelona, Mart\'{i} i Franqu\`{e}s 1, E08028 Barcelona, Spain
10. ICREA, Pg. Lluis Companys 23, 08010 Barcelona, Spain
11. Argelander-Institüt für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
12. Department of Physics, University of Oxford, Keble Road, Oxford OX13RH, UK
13. Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG, UK
PP 019030
Intrinsic and observed dual AGN fractions from major mergers
(1) Universitat de Barcelona, (2) ICCUB, (3) IAA, (4) IAC, (5) ULL
PP 019029
The VLT-FLAMES Tarantula Survey. XXX. Red stragglers in the clusters Hodge 301 and SL 639.
(1) Instituto de Astrof\'isica de Canarias, E-38205 La Laguna, Tenerife, Spain
(2) Universidad de La Laguna, Dpto. Astrof\'isica, E-38206 La Laguna, Tenerife, Spain
(3) ESA, European Space Astronomy Centre, Apdo. de Correos 78, E-28691 Villanueva de la Cañada, Madrid, Spain
(4) UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK
(5) Argelander-Institut für Astronomie der Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
(6) Lennard-Jones Laboratories, Keele University, Staffordshire, ST5 5BG, United Kingdom
(7) School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, United Kingdom
(8) Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United Kingdom
(9) Zentrum f\"{u}r Astronomie der Universit\"{a}t Heidelberg, Astronomisches Rechen-Institut, M\"{o}nchhofstr. 12-14, 69120 Heidelberg, Germany
(10) Heidelberger Institut f\"{u}r Theoretische Studien, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany
(11) Departamento de F\'isica Te\'orica e Experimental, Universidade Federal do Rio Grande do Norte, CP 1641, Natal, RN, 59072-970, Brazil
(12) Institute of astrophysics, KU Leuven, Celestijnlaan 200D, 3001, Leuven, Belgium
(13) Anton Pannenkoek Institute for Astronomy, University of Amsterdam, 1090 GE Amsterdam, The Netherlands
PP 019028
Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
Several institutions across Europe (including IAC/ULL)
PP 019027
Asteroseismology of massive stars with the TESS mission: the runaway Beta Cep pulsator PHL 346 = HN Aqr
(1) Nicolaus Copernicus Astronomical Center, Poland
(2) IAC/ULL, Spain
PP 019026
The weakening outburst of the young eruptive star V582 Aur
(1) Konkoly Observatory, Budapest, Hungary
(2) Eötvös Loránd University, Budapest, Hungary
(3) IAC
(4) Astrophysics Department ULL
PP 019025
The outbursting protostar 2MASS 22352345+7517076 and its environment
(1) Kinkily Observatory, Research Centre for Astronomy and Earth Sciences, Hungary
(2) IAC
(3) Directorate of Science, ESTEC–ESA
PP 019024
Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
(1) Universität Wien, Austria,
(2) IAC / ULL
PP 019023
Diagnostic potential of the Ca II 8542A line for solar filaments
(1) Instituto de Astrofisica de Canarias
(2) Universidad de La Laguna
(3) Stockholm University
PP 019022
Strong lensing reveals jets in a sub-microJy radio quiet quasar
(1) Jodrell Bank Centre for Astrophysics, School of Physics & Astronomy, University of Manchester,
(2) STAR Institute,
(3) ASTRON, Netherlands Institute for Radio Astronomy,
(4) Kapteyn Astronomical Institute,
(5) Instituto de Astrofísica de Canarias,
(6) Departmento de Astrofísica, Universidad de La Laguna
PP 019021
Detection and characterization of an ultra-dense sub-Neptunian planet orbiting the Sun-like star K2-292
(1) Instituto de Astrofísica de Canarias (IAC), 38205 La Laguna, Tenerife
(2) Departamento de Astrofísica, Universidad de La Laguna (ULL),
38206, La Laguna, Tenerife, Spain
PP 019020
Spectral analysis of the barium central star of the planetary nebula Hen 2-39
(1) ESO, Germany; (2) Tubingen, Germany, (3) IAC, (4) ULL
PP 019019
Observations of tides and circularization in red-giant binaries from Kepler photometry
(1) IAC/ULL (2) CEA, Paris-Saclay (3) Univ. Vienna, Austria
PP 019018
Exploring circumstellar effects on the lithium and calcium abundances in massive Galactic O-rich AGB stars
(1) Instituto de Astrofísica de Canarias (IAC), (2) Universidad de La Laguna (ULL), (3) Laboratoire Univers et Particules de Montpellier, (4) Consejo Superior de Investigaciones Científicas (CSIC), (5) Monash Centre for Astrophysics, (6) Konkoly Observatory
PP 019017
Title: Formation of S0 galaxies through mergers. Morphological properties: tidal relics, lenses, ovals, and other inner components
1. IAC ; 2. ULL; 3. MPIA Heidelberg; 4. UNAM-Ensenada.
PP 019016
The ALHAMBRA survey: 2D analysis of the stellar populations in massive early-type galaxies at z < 0.3
(1) CEFCA. Teruel (2) IAC (3) ULL
PP 019015
Extreme HBL behavior of Markarian 501 during 2012
(1) ETH Zurich; (2) Instituto de Astrofísica de Canarias
PP 019014
Constraining Metallicity Dependent Mixing and Extra Mixing using [C/N] in Alpha-Rich Field Giants
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019013
First stellar spectroscopy in Leo P
(1) UK Astronomy Technology Centre, Royal Observatory Edinburg
(2) IAC/ULL
PP 019012
Title:Diverse Variability of O and B Stats Revealed from 2-minute Cadence Light Curves in Sectors 1 and 3 of the TESS Mission: Selection of an Asteroseismic Sample
[1] KU Leuven, [2] IAC/ULL + others
PP 019011
Title:The Fornax 3D project: Unveiling the thick disk origin in FCC 170; possible signs of accretion
(1) Instituto de Astrofísica de Canarias, (2) Depto. Astrofísica, Universidad de La Laguna, (3) Astrophysics Research Institute, Liverpool John Moores University, (4) Centre for Astrophysics Research, University of Hertfordshire, (5) European Southern Observatory, (6) INAF-Osservatorio Astronomico di Capodimonte, (7) Dipartimento di Fisica e Astronomia 'G. Galilei', Università di Padova, (8) INAF-Osservatorio Astronomico di Padova, (9) Sterrewacht Leiden, Leiden University, (10) Max-Planck-Institut fuer extraterrestrische Physik, (11) Max-Planck Institut fuer Astronomie, (12) Department of Physics and Astronomy, Macquarie University, (13) Leibniz-Institut für Astrophysik Potsdam, (14) Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama, (15) Sterrenkundig Observatorium, Universiteit Gent
PP 019010
The MUSE Atlas of Disks (MAD): Resolving Star Formation Rates and Gas Metallicities on < 100pc Scales
(1)Department of Physics, ETH,
(2)Leibniz-Institut fur Astrophysik Potsdam (AIP),
(3)Subaru Telescope, National Astronomical Observatory of Japan,
(4)Leiden Observatory,
(5) Instituto de Astrofísica e Ciências do Espaco,
(6) Instituto de Astrofísica de Canarias,
(7) Departamento de Astrofísica, Universidad de La Laguna,
(8) Dept. of Physics & Astronomy, University of Victoria,
(9)Astronomy Centre, Department of Physics and Astronomy, University of Sussex,
(10)Jeremiah Horrocks Institute, University of Central Lancashire,
(11)Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon,
(12)Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA
PP 019009
The MUSE Atlas of Disks (MAD): Resolving Star Formation Rates and Gas Metallicities on < 100pc Scales
(1)Department of Physics, ETH,
(2)Leibniz-Institut fur Astrophysik Potsdam (AIP),
(3)Subaru Telescope, National Astronomical Observatory of Japan,
(4)Leiden Observatory,
(5) Instituto de Astrofísica e Ciências do Espaco,
(6) Instituto de Astrofísica de Canarias,
(7) Departamento de Astrofísica, Universidad de La Laguna,
(8) Dept. of Physics & Astronomy, University of Victoria,
(9)Astronomy Centre, Department of Physics and Astronomy, University of Sussex,
(10)Jeremiah Horrocks Institute, University of Central Lancashire,
(11)Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon,
(12)Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA
PP 019008
Title:Discovery of disc truncations above the galaxies' mid-plane in Milky Way-like galaxies
1. Instituto de Astrofísica de Canarias (IAC), La Laguna, 38205, Spain
2. Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38200, La Laguna, Spain
3. Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool, L3 5RF, UK
PP 019007
Identifying Sagittarius Stream Stars By Their APOGEE Chemical Abundance Signatures
Several institutions from North and South America and Europe (including IAC and ULL)
PP 019006
Discovery of stars surrounded by iron dust in the LMC
(1) Univ. Roma Tre; (2) IAC-ULL; (3) OAR-INAF; (4) ASI-Roma; (5) Nordita-KTH
PP 019005
Spiral structure in barred galaxies. Observational constraints to spiral arm formation mechanisms
1. Instituto de Astrofísica de Canarias 2. Departamento de Astrofísica, Universidad de La Laguna 3.Astrophysics Institute, Liverpool John Moores University (UK) 4. Research Centre for Astronomy, Academy of Athens, Greece.
PP 019004
Disentangling the spatial substructure of Cygnus OB2 from Gaia DR2
(1) Instituto de Astrofisica de Canarias (2) Departamento de Astrofisica, ULL
(3) Keele University (4) University of Hertfordshire (5) ESA, European Space Astronomy Centre.
PP 019003
Quantifying star formation activity in the inner 1kpc of local MIR bright QSOs
(1) UNAM, (2) KASSI, (3) INAOE, (4) CAB, (5) STSI, (6) IAC, (7) ULL, (8) NASA/SOFIA
PP 019002
Radial velocities in the outermost disk toward the anticenter
(1) IAC, (2) ULL, (3) Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy, (4) Istituto dei Sistemi Complessi CNR, Rome, Italy, (5) INFN Unit Rome 1, Dipartimento di Fisica, Universitá di Roma “Sapienza”, Rome, Italy, (6) Argelander-Institut für Astronomie, Bonn, Germany
PP 019001
Title:SOFIA/FORCAST resolves 30 - 40 micron extended dust emission in nearby active galactic nuclei
(1) UTSA, (2) IAC, (3) ULL