Preprints in 2012
PP 012064
Probing nuclear activity versus star formation at z~0.8 using near-infrared multi-object spectroscopy
(1)IAC, (2)ULL, (3)IFCA, (4)Augusto González Linares Senior Research Fellow
PP 012063
Far- and mid-infrared spectroscopy of complex organic matter of astrochemical interest: coal, heavy petroleum fractions, and asphaltenes
(1) INAF; (2) ACR; (3) IAC; (4) ULL; (5) CSIC
PP 012062
Determination of the Integrated Molar Absorptivity and Molar Extinction Coefficient of Hydrogenated Fullerenes
a Istituto Nazionale di Astrofisica – Osservatorio Astrofisico di
Catania, Catania, Italy
b Actinium Chemical Research, Rome, Italy
c Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
d Departamento de Astrofısica, Universidad de La Laguna (ULL), La
Laguna, Spain
e Consejo Superior de Investigaciones Científicas, Madrid, Spain
PP 012061
FT-IR SPECTRA OF FULLERENES C76, C78 and C84 AT TEMPERATURES COMPRISED BETWEEN -180°C AND +250°C
1Actinium Chemical Research srl, Via Casilina 1626/A, 00133 Rome, Italy.
2National Center for Astronomy, KACST, P.O. box 6086, Riyadh 11442, Saudi Arabia
3Instituto de Astrofisica de Canarias, Via Láctea s/n E-38200, La Laguna, Tenerife, Spain,
4Departamento de Astrofısica, Universidad de La Laguna (ULL), E-38205 La Laguna, Spain
PP 012060
Solid state radiolysis of non-proteinaceus amino acids in vacuum:astrochemical implications
F. Cataldo
Istituto Nazionale di Astrofisica, Osservatorio Astrofisica
di Catania, Via S. Sofia 78, 95123 Catania, CT, Italy
F. Cataldo (&)
Lupi Chemical Research, Via Casilina 1626/A, 00133 Rome,
Italy
e-mail: franco.cataldo@fastwebnet.it
G. Angelini
Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300,
00016 Monterotondo Stazione, Rome, Italy
Y. Hafez
National Center for Astronomy, KACST, P.O. Box 6086,
Riyadh 11442, Saudi Arabia
S. Iglesias-Groth
Instituto de Astrofisica de Canarias, Via Lactea s/n,
38200 La Laguna, Tenerife, Spain
123
PP 012059
Early-type Galaxies with Tidal Debris and Their Scaling Relations in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
Various incl IAC & ULL
PP 012058
A unified picture of breaks and truncations in spiral galaxies from SDSS and S^{4}G imaging
IAC & ULL and others
PP 012057
Breaks in Thin and Thick Disks of Edge-on Galaxies Imaged in the Spitzer Survey Stellar Structure in Galaxies (S4G)
Univ. Oulu and others (incl. IAC & ULL)
PP 012056
Spectral Energy Distributions of Type 1 Active Galactic Nuclei in the COSMOS Survey. I. The XMM-COSMOS Sample
Harvard CfA, et al. (including IAC)
PP 012055
Hα Kinematics of S4G spiral galaxies I. NGC 864
IAC, Laboratoire d'Astrophysique de Marseille, ESO, NRAO, etc.
PP 012054
The JCMT Nearby Galaxies Legacy Survey VIII. CO data and the L(CO3-2)-L(FIR) correlation in the SINGS sample
Varias (incluyendo Instituto de Astrofísica de Canarias)
PP 012053
Hydrogen volume densities in nearby galaxies I - an automated approach
Université Laval, Québec; Instituto de Astrofísica de Canarias; Centro de Radioastronomía y Astrofísica (CRyA), Universidad Nacional Autónoma de México; Instituto de Astrofísica de Canarias
PP 012052
Structure of Abell 1995 from optical and X-ray data: a galaxy cluster with an elongated radio halo
(1) Fundacion Galileo Galilei - TNG (INAF)
(2) Physics Dep. Univ Trieste (Italy)
(3) Trieste Observatory (Italy)
(4) DA-ULL
(5) IAC
PP 012051
The hot R Coronae Borealis star DY Centauri is a binary
1)IIA; (2) The W.J. McDonald Observatory-UT; (3) IAC; (4) ULL; (5) Armagh Observatory; (6) University of Nebraska
PP 012050
Dark Matter, Magnetic Fields, and the Rotation Curve of the Milky Way
(1) UGR, (2) IAC and ULL
PP 012049
Planck Intermediate Results. IV. The XMM-Newton validation programme for new Planck galaxy clusters
IAC and others
PP 012048
Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal
IAC and others
PP 012047
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
(1) MPE, (2) IAC, and others
PP 012046
ANALYTIC APPROXIMATE SEISMOLOGY OF PROPAGATING MHD WAVES IN THE SOLAR CORONA
(1) Centre for Mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium; (2) Solar Physics Group, Departament de Fisica, Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain; (3) Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38205 La Laguna, Tenerife, Spain; (4) Departamento de Astrofisica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 012045
High-resolution optical spectroscopy of DY Cen: diffuse interstellar bands in a proto-fullerene circumstellar environment?
(1) Instituto de Astrofisica de Canarias; (2) Departamento de Astrofisica-ULL; (3) Indian Institute of Astrophysics; (4) The W.J. McDonald Observatory
PP 012044
Evolutionary paths among different red galaxy types at 0.3 < z < 1.5 and the late buildup of massive E-S0’s through major mergers
1-Instituto de Astrofísica de Canarias, C/ Vía Láctea, E-
38200, La Laguna, Canary Islands, Spain
2-Departamento de Astrofísica, Universidad de La Laguna,
Avda. Astrofísico Fco. Sánchez, E-38200, La Laguna,
Canary Islands, Spain
3-Departamento de Astrofísica, Facultad de CC. Físicas,
Universidad Complutense de Madrid, E-28040 Madrid,
Spain
4-Isaac Newton Group of Telescopes, Apartado 321, E-
38700, Santa Cruz de La Palma, Canary Islands, Spain
5-Centro de Estudios de Física del Cosmos de Aragón, E-
44001, Teruel, Spain
6-Instituto de Astrofísica de Andalucía, IAA-CSIC, Apdo.
3044, E-18080 Granada, Spain
7-Max-Planck-Institut für Extraterrestrische Physik,
Giessen-bachstrasse, D-85748, Garching, Germany
8-Universitätssternwarte, Scheinerstrasse 1, D-81679,
München, Germany
9-Department of Astronomy, 477 Bryant Space Center,
University of Florida, Gainesville, FL, USA
10-Associate Astronomer at Steward Observatory, The
University of Arizona, USA
PP 012043
An Infrared Study of Fullerene Planetary Nebulae
(1) IAC; (2) ULL; (3) UAM; (4) ESAC-ESA; (5) CSIC; (6) NOAO; (7) INAF-Osservatorio Astrofisico di Catania; (8) Actinium Chemical Research
PP 012042
Peaks in the CMBR power spectrum. I. Mathematical analysis of the associated real space features
(1) IAC, (2) ULL, (3) Istituto dei Sistemi Complessi CNR, Via dei Taurini 19, 00185 Rome, Italy, (4) IMT Institute of Advanced Studies, Piazza S. Ponziano 6, 55100 Lucca, Italy, (5) London Institute of Mathematical Science, 35a South St,
London W1K 2XF, UK
PP 012041
The long bar as seen by the VVV survey: I. Colour-magnitude diagrams
(1) Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, (2) IAC, (3) ULL, (4) FCUL, Lisboa, Portugal, (5) Laboratório Nacional de Astrofísica MCTI, Brazil, (6) Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, (7) Vatican Observatory, (8) Centre for Astrophysics Research, University of Hertfordshire, U.K.
PP 012039
PKS0347+05: a radio-loud/radio-quiet double AGN system triggered in a major galaxy merger
(1) University of Sheffield, (2) IAC, (3) ULL, (4) ASTRON
PP 012038
Anomalous circular polarization profiles in the He I 1083.0 nm multiplet from solar spicules
IAC
PP 012037
Resolving the internal magnetic structure of the solar network
(1) Instituto de Astrofísica de Canarias, (2) Instituto de Astrofísica de Andalucía, (3) Max-Planck-Institut für Sonnensystemforschung, (4) Kiepenheuer-Institut für Sonnenphysik
PP 012036
Resolving the internal magnetic structure of the solar network
(1) Instituto de Astrofísica de Canarias, (2) Instituto de Astrofísica de Andalucía, (3) Max-Planck-Institut für Sonnensystemforschung, (4) Kiepenheuer-Institut für Sonnenphysik
PP 012035
Analysis of the CN and CH molecular band strengths in stars of the open cluster NGC 6791
(1) Instituto de Astrofísica de Canarias, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, Spain
PP 012034
Mapping Luminous Blue Compact Galaxies with VIRUS-P: morphology, line ratios and kinematics
(1) Leibniz-Institut fuer Astrophysik, Potsdam, Germany; (2) IAC and ULL, Tenerife, Spain; (3) Centro de Astrofisica, Universidade do Porto, Portugal
PP 012033
Short-lived radioactivity in the early Solar System: the Super-AGB star hypothesis
(1) MoCa, Monash University; (2) Mt. Stromlo Obs, ANU; (3) CAS, Swinburne University; (4) CSIRO/MSE; (5) IAC-ULL; (6) ULB
PP 012032
The importance of galaxy interactions in triggering type II quasar activity
(1) University of Sheffield, (2) IAC, (3) ULL, (4) IAA, (5) CAB
PP 012031
Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters: Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266
Instituto de Astrof\'isica de Canarias, La Laguna, Tenerife, Spain
Departamento de Astrof\'isica, Universidad de La Laguna, Tenerife, Spain
PP 012030
Kinetic power of quasars and statistical excess of MOJAVE superluminal motions
(1) IAC, (2) ULL, (3) Dept. d'Astronomia i Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
PP 012029
The Chemical composition of the post-AGB F-supergiant CRL 2688
(1) National Astronomical Observatory of Japan; (2) Aryabhatta Research Institute of Observational Sciences; (3) Indian Institute of Astrophysics; (4) Herschel Science Centre, ESAC; (5)IAC; (6) ULL; (7) CSIC
PP 012028
The stellar and sub-stellar IMF of simple and composite populations
(1) Argelander-Institut fuer Astronomie, (2) University of St Andrews, (3) IAC, (4) Institute of Astronomy, Cambridge, (5) Institut de Planetologie et dAstrophysique de Grenoble
PP 012027
Field O stars: formed in situ or as runaways?
(1) Sternberg Astronomical Institute, Russia, (2) Isaac Newton Institute of Chile, Russia, (3) IAC, (4) University of St Andrews, (5) Argelander-Institut fuer Astronomie, Germany
PP 012026
Probing the Nuclear and Circumnuclear Activity of NGC1365 in the Infrared
(1)Instituto de Física de Cantabria, (2)Augusto González Lineres Senior Research Fellow, (3)IAC, (4)Departamento de Astrofísica, Universidad de La Laguna
PP 012025
ON THE RADICAL ANION SPECTRA OF FULLERENES C60 AND C70
1Istituto Nazionale di Astrofisica. Osservatorio Astrofisico di Catania, Via S. Sofia 78,
95123 Catania, Italy.
2Actinium Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy.
3Instituto de Astrofísica de Canarias (IAC), Via Lactea s/n, E-38200 La Laguna, Tenerife,
Spain.
4CSIC, Spain.
PP 012024
On the Radical Cation Spectra of Fullerenes and Fulleranes. Part 1: C60, C70,C76, C78 and C84
1Istituto Nazionale di Astrofisica – Osservatorio Astrofisica di Catania,
Catania, Italy
2Actinium Chemical Research, Rome, Italy
3Instituto de Astrofisica de Canarias, Tenerife, Spain
4Universidad de La Laguna, Tenerife, Spain
5Consejo Superior de Investigaciones Cientificas, Spain
PP 012023
On the Radical Cation Spectra of Fullerenes and Fulleranes. Part 2: C60H36, C70H38, C60H18 and C60Hx/C70Hy Mixture
1Istituto Nazionale di Astrofisica – Osservatorio Astrofisica di Catania,
Catania, Italy
2Actinium Chemical Research, Rome, Italy
3Instituto de Astrofisica de Canarias, Tenerife, Spain
4Universidad de La Laguna, Tenerife, Spain
5Consejo Superior de Investigaciones Cientificas, Spain
PP 012022
Unusual high frequency oscillations in the Kepler delta Scuti star KIC4840675
(1) SAAO, (2) University of Texas, (3) INAF - OA Catania, (4) Universidade do Porto, (5) Nicolaus Copernicus Astronomical Center, Warsaw, (6) Wroclaw University, (7) University of Central Lancashire, (8) Keele University, (9) Konkoly Observatory, (10) IAC, (11) ULL, (12) SETI Institute/NASA Ames, (13) Orbital Sciences Corporation/NASA Ames
PP 012021
Accurate fundamental parameters and detailed abundance patterns from spectroscopy of 93 solar-type Kepler targets
(1) Aarhus University, (2) Observatoire de Paris, (3) Yale University, (4) Keele University, (5) University of Birmingham, (6) University of London, (7) University of Sydney, (8) University Aix-Marseille & CNRS, (9) University of Wroclaw, (10) IAC, (11) ULL, (12) University of Amsterdam, (13) HAO, Boulder, (14) IAS, (15) Universidade do Porto, (16) CEA, Saclay, (17) Canadian Space Agency, (18) Iowa State University, (19) SETI/NASA AMES, (20) NASA AMES
PP 012020
A multisite photometric study of two unusual Beta Cep stars: the magnetic V2052 Oph and the massive rapid rotator V986 Oph
(1) Copernicus Astronomical Center, Warsaw, (2) Australian National University, Canberra, (3) IAC, (4), ULL, (5) ULG, Liege, (6) KULeuven, (7) Observatoire de Paris, (8) University of the North-West, Mmabatho, (9) University Vienna, (10) IAA, (11) Homi Bbabha Centre for Science Education, Mumbai, (12) Akdeniz University, Antalya, (13) Tubitak observatory
PP 012019
Rayleigh-Taylor instability in partially ionized compressible plasmas
(1) Instituto de Astrofísica de Canarias, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de la Laguna, Tenerife, Spain
(3) Centre for Plasma Astrophysics, Department of Mathematics, KU Leuven, Belgium
(4) Universitat de les Illes Balears, Palma de Mallorca, Spain
PP 012018
The nature of dust in compact Galactic planetary nebulae from Spitzer spectra
(1) NOAO; (2) IAC-ULL; (3) ESA-ESAC; (4) Spitzer Science Center-CIT; (5) UAM; (6) INSA-ESAC
PP 012017
Ionized gas diagnostics from protoplanetary discs in the Orion Nebula and the abundance discrepancy problem
(1) Departamento de Astronomía y Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Santiago, Chile, (2) Institute for Astronomy, Honolulu, HI, USA, (3) Instituto de Astrofísica de Canarias, Tenerife, Spain, (4) Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain, (5) Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Campus Morelia, Michoacán, México, (6) European Southern Observatory, Garching bei München, Germany
PP 012016
The Nuclear Infrared Emission of Low-Luminosity Active Galactic Nuclei
(1) Gemini Observatory, (2) University of Florida, (3) Instituto de Física de Cantabria, (4) IAC, (5) Centro de Astrobiología (CSIC/INTA), (6) University of Kentucky, (7) INAOE, (8) University of Oxford, (9) SOKENDAY, Tokyo
PP 012015
INFRARED SPECTROSCOPY OF HYDROGENATED FULLERENES (FULLERANES) AT EXTREME TEMPERATURES
1Instituto de Astrofísica de Canarias, Vía Lactea s/n, E-38200, La Laguna, Tenerife, Spain,
2 Departamento de Astrofísica. Universidad de La Laguna. E-38200, La Laguna, Tenerife, Spain
3Istituto Nazionale di Astrofisica – Osservatorio Astrofisica di Catania, Via S. Sofia 78, 95123, Italy
4Actinium Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy
5CSIC, Consejo Superior de Investigaciones Cientificas, Madrid, Spain
PP 012014
Satellites around massive galaxies since z~2
(1) IAC, (2) UCM, (3) Steward Observatory-University of Arizona, (4) CEFCA, (5) UCO/Lick Observatory-University of California
PP 012013
Young ages and other intriguing properties of massive compact galaxies in the Local Universe
(1) IAC, (2) ULL, (3) Universidad Autónoma de Madrid, (4) Universidad de Valencia
PP 012011
Abell 1758N from an optical point of view: new insights on a merging cluster with diffuse radio emission
(1) Fundación Galileo Galilei - INAF (TNG), La Palma, Spain
(2) Dpto. de Física de la Univ. degli Studi di Trieste.
(3) INAF - Osservatorio Astronomico di Trieste, Trieste, Italy
(4) IAC
(5) ULL
PP 012010
Heavy element nucleosynthesis in the brightest Galactic Asymptotic Giant Branch stars
(1) Research School of Astronomy and Astrophysics, Mt. Stromlo Observatory; (2) IAC; (3) ULL; (4) Monash Centre for Astrophysics
PP 012009
The JCMT Nearby Galaxies Legacy Survey VII: Hα imaging and massive star formation properties
IAC, ULL, McMaster, UWO, CfA, Queen's
PP 012008
The S4G perspective on circumstellar dust extinction of AGB stars in M100
MPIA, IAC, ULL, etc.
PP 012007
Anomalous Cepheids in the Large Magellanic Cloud: Insight on their origin and connection with the star formation history
(1)INAF-Osservatorio Astronomico di Bologna; (2) IAC; (3) ULL
PP 012006
Rubidium, zirconium, and lithium production in intermediate-mass asymptotic giant branch stars
(1) University of Utrecht; (2) Monash Centre for Astrophysics; (3) Research School of Astronomy and Astrophysics, Mt. Stromlo Observatory; (4) IAC; (5), ULL
PP 012005
High resolution spectroscopy of the high velocity hot post−AGB star LS III +52 24 (IRAS 22023+5249)
(1) Indian Institute of Technology; (2) IAC; (3) ULL; (4) National Astronomical Observatory of Japan; (5) Aryabhatta Research Institute of Observational Sciences; (6) CSIC; (7) Herschel Science Centre, ESAC
PP 012004
Environmental effects on the bright end of the galaxy luminosity function in galaxy clusters
(1) IAC
(2) Dpto. de Astrofisica, ULL
(3) Dipartimento di Fisica. Universita degli Studi di Trieste (Italy)
(4) Osservatorio Astronomico di Trieste (Italy)
(5) Fundacion Galileo Galilei - INAF (Spain)
PP 012003
Exploring the effects of high-velocity flows in abundance determinations in H II regions. Bidimensional spectroscopy of HH 204 in the Orion Nebula
(1) IAC, (2) Dept. Astrofisica ULL, (3) Departamento de Astronomia y Astrofisica Pontificia Universidad Catolica de Chile
PP 012002
Variable Stars in the Cetus dSph Galaxy: Population Gradients and Connections with the Star Formation History
(1) IAC; (2) Departamento de Astrofísica, ULL; (3) Institute for Astronomy, University of Edinburgh; (4) INAF-Osservatorio Astronomico di Bologna ; (5)
Universitá di Roma Tor Vergata; (6) INAF-Osservatorio Astronomico di Roma; (7) INAF-Osservatorio Astronomico di Teramo; (8) Minnesota Institute for strophysics; (9)NRC Herzberg Institute for Astrophysics