Preprints in 2013
PP 013093
The VLT-FLAMES Tarantula Survey. XIII: On the nature of O Vz stars in 30 Doradus
(1) IAC, (2) ULL
PP 013092
Unveiling the Structure of Barred Galaxies at 3.6 $μ{ m m}$ with the Spitzer Survey of Stellar Structure in Galaxies (S$^4$G): I. Disk Breaks
(1) Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea; thkim@astro.snu.ac.kr
(2) European Southern Observatory, Casilla 19001, Santiago 19, Chile
(3) National Radio Astronomy Observatory/NAASC, 520 Edgemont Road, Charlottesville, VA 22903, USA
(4) The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101, USA
(5) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
(6) Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 013091
The multi-wavelength polarization of Cygnus X–1
(1)Instituto de Astrof´ısica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain, (2)Departamento de Astrof´ısica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain, (3)New York University Abu Dhabi, P.O. Box 129188, Abu Dhabi, United Arab Emirates
PP 013090
ARRAKIS: Atlas of Resonance Rings As Known In the S4G
(1) University of Oulu, Astronomy Division, Department of Physics, P.O. Box 3000, FIN-90014, Finland
(2) Finnish Centre of Astronomy with ESO (FINCA), University of Turku, Va ̈isa ̈la ̈ntie 20, FI-21500, Piikkio ̈, Finland
(3) Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon 305-348, Republic of Korea
(4) Instituto de Astrof ́ısica de Canarias, E-38205 La Laguna, Tenerife, Spain
(5) Departamento de Astrof ́ısica, Universidad de La Laguna, E-38200, La Laguna, Tenerife, Spain
PP 013087
Li depletion in solar analogues with exoplanets: Extending the sample
(1) CAUP, Universidade do Porto, (2) IAC, (3) CGUC, University of Coimbra, (4) Observatoire de Geneve
PP 013086
NGC1277: a massive compact relic galaxy in the nearby Universe
(1) Instituto de Astrofisica de Canarias
(2) Subaru Telescope
(3) Isaac Newton Group of Telescopes
(4) Universidad Autonoma de Madrid
PP 013083
Shock Excited Molecules in NGC 1266: ULIRG conditions at the center of a Bulge Dominated Galaxy
Univ. of Toledo (USA), IAC, ULL, etc.
PP 013082
Spectroscopic and physical parameters of Galactic O-type stars. II. Observational constraints on projected rotational and extra broadening velocities as a function of fundamental parameters and stellar evolution
IA-NOA, USM, IAC, IfA
PP 013081
The IACOB project: I. Rotational velocities in Northern Galactic O and early B-type stars revisited. The impact of other sources of line-broadening
IAC
PP 013080
The circumnuclear environment of NGC613: a nuclear starburst caught in the act?
(1) IAC, (2) ULL, (3) ESA, (4) MPIA, (5) Observatoire Astronomique de Strasbourg, (6) Australian Astronomical Observatory
PP 013079
Nuclear star formation activity and black hole accretion in nearby Seyfert galaxies
(1)CAB, (2)IFCA, (3)Universidad de Cantabria, (4)IAC, (5)ULL, (6)University of Copenhagen, (7)University of Oxford, (8)Gemini North, (9)Spitzer Science Center, (10)Gemini South, (11)INAOE, (12)UTSA
PP 013078
Embedded Star Formation in S4G Galaxy Dust Lanes
1) Vassar College, Dept. of Physics and Astronomy, Poughkeepsie, NY 12604
2) IBM Research Division, T.J. Watson Research Center, Yorktown Hts., NY 10598
3) Instituto de Astrofísica de Canarias, Vía Láctea s/n 38205 La Laguna, Spain
4) Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Spain
PP 013077
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function
1 - Instituto de Astrofísica de Canarias
2 - Departamento de Astrofísica, ULL
3 - Max-Planck Institute für extraterrestrische Physik
PP 013076
Long-term monitoring, time delay and microlensing in the gravitational lens system Q0142-100
Instituto de Astrofísica de Canarias-Universidad de La Laguna
Universidad de Valencia
PP 013075
Radio observations of extreme ULXs: revealing the most powerful ULX radio nebula ever or the jet of an intermediate-mass black hole?
(1) Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain
(2) Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain
(3) Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK
(4) Max Planck Institute for Radio Astronomy, Auf dem Hügel 69, D-53121 Bonn, Germany
PP 013074
Milliarcsec-scale radio emission of ultraluminous X-ray sources: steady jet emission from an intermediate-mass black hole?
(1)Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain
(2)Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain
(3)Max Planck Institute for Radio Astronomy, Auf dem Hügel 69, D-53121 Bonn, Germany
(4)Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, NSW 2006, Australia
(5)Department of Physics, University of Alberta, 11322-89 Avenue, Edmonton, Alberta, T6G 2G7, Canada
PP 013073
The rotation rates of massive stars: How slow are the slow ones?
(1) USM, (2) IAC, (3) ULL, (4) IA/NOA
PP 013072
Deep high spectral resolution spectroscopy and chemical composition of ionized nebulae.
(1) IAC, (2) Dep. Astrofísica, ULL, (3) PUC, Chile
PP 013071
Gamma Radiolysis of C60 fullerene in water and water/ammonia mixtures: relevance of fullerene fate in ices of interstellar medium
Instituto de Astrofısica de Canarias, Via Lactea s/n,
38205 La Laguna, Spain
Departamento de Astrofısica, Universidad de La Laguna (ULL),
38206 La Laguna, Spain
National Center for Astronomy, KACST, P.O. Box 6086,
Riyadh 11442, Saudi Arabia
Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300,
00016 Monterotondo Stazione Rome, Italy
INAF-Osservatorio Astrofisico di Catania, Via S. Sofia 78,
95123 Catania, Italy
Actinium Chemical Research srl, Via Casilina 1626/A00133. Rome, Italy
PP 013070
INTERLOCKING RESONANCE PATTERNS IN GALAXY DISKS.
1. Instituto de Astrofísica de Canarias,jfont@iac.es, jeb@iac.es, serroz@iac.es.
2. Departamento de Astrofísica. Universidad de La Laguna, Tenerife, Spain.
3. Consejo Superior de Investigaciones Científicas, Spain.
4 Max-Plack.Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany:
querejeta@mppia.de
5. Laboratoire d’Astrophysique de Marseille, Université d’Aix-Marseille & CNRS, UMR7326, 38 rue
F. Juliot-Curie, 13388 Marseille Cedex 13, France: benoit.epinat@oamp.fr.
6 Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton
Wharf, Birkenhead, CH41 ILD, UK: paj@astro.livjm.ac.uk
7 Department of Astronomy, University of Stockholm, AlbaNova, 10691, Stockholm, Sweden
8 Instituto de Astrofísica de Andalucia, CSIC, Apdo. 3004, 18080 Granada, Spain: blasco@iaa.es
9 Departamento de Física Teórica y del Cosmos, Universidad de Granada, Spain: isa@ugr.es
PP 013069
The role of the accretion disk, dust, and jets in the IR emission of low-luminosity AGN
(1) Gemini Observatory, Northern Operations Center, (2) IAC, (3) ULL, (4) Gemini Observatory, Southern Operations Center, (5) IFCA, CSIC
PP 013068
The galaxy-wide IMF of dwarf late-type to massive early-type galaxies
(1) IAC, (2) ULL, (3) HISKP, (4) AIfA
PP 013067
Massive star formation in galaxies with excess UV emission
(1)Instituto de Astrof ́ısica de Canarias, V ́ıa La ́ctea s/n 38205 La Laguna, Spain
(2)Departamento de Astrof ́ısica, Universidad de La Laguna, 38206 La Laguna, Spain
(3)School of Physics and Astronomy, University of St Andrews, North Haugh, Fife KY16 9SS St Andrews, UK
(4)Department of Astronomy, University of Wisconsin - Madison, 475 N. Charter St., Madison, WI, 53706, USA
(5)Department of Astronomy & Astrophysics, The Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, USA
(6)Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
(7)The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA
PP 013066
THE ACS LCID PROJECT. IX. IMPRINTS OF THE EARLY UNIVERSE IN THE RADIAL VARIATION OF THE STAR FORMATION HISTORY OF DWARF GALAXIES.
(1) IAC, (2) ULL, (3) MIA-UofM, (4) INAF-Teramo, (5) IA, U. of Edinburgh, (6) Institut für Astronomie, ETH Zürich, (7) DAO, Victoria, (8) University of Tasmania, (9) Raytheon, Tucson
PP 013065
The VLT-FLAMES Tarantula Survey XII. Rotational velocities of the single O-type stars
(1) Astronomical Institute Anton Pannekoek (2) IAC (3) ULL
PP 013064
Morphological Parameters of Spitzer Survey of Stellar Structure in Galaxies (S4G)
(1) European Space Agency Research Fellow (ESTEC), Ke- plerlaan 1, 2200 AG Noordwijk, The Netherlands
(2) National Radio Astronomfy Observatory/NAASC, 520 Edgemont Road, Charlottesville, VA 22903, USA
(3) Astronomy Division, Department of Physical Sciences, FIN- 90014 University of Oulu, P.O. Box 3000, Oulu, Finland
(4) Max-Planck-Institut fu ̈r Astronomie / K ̈onigstu ̈hl 17 D- 69117, Heidelberg, Germany
(5) Spitzer Science Center, 1200 East California Boulevard, Pasadena, CA 91125, USA
(6) Spitzer Science Center, Mail Stop 220-6, 1200 East Califor- nia Boulevard, Pasadena, CA 91125, USA
(7) Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA
(8) Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
(9) Departamento de Astrof ́ısica, Universidad Complutense de Madrid, 28040 Madrid, Spain
(10) The Observatories of the Carnegie Institution of Washing- ton, 813 Santa Barbara Street, Pasadena, CA 91101, USA
(11) Astronomy Program, Department of Physics and Astron- omy, Seoul National University, Seoul 151-742, Republic of Ko- rea
(12) Finnish Centre of Astronomy with ESO (FINCA), Univer- sity of Turku, Vislntie 20, FI-21500, Piikki, Finland
(13) European Southern Observatory, Casilla 19001, Santiago 19, Chile
(14) Instituto de Astrof ́ısica de Canarias, V ́ıa La ́ctea s/n 38205 La Laguna, Spain
(15) Departamento de Astrof ́ısica, Universidad de La Laguna, Avda. Astrof ́ısico Francisco S ́anchez s/n 38206 La Laguna, Spain
(16) Aix Marseille Universit ́e, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388, Marseille, France
PP 013063
Long-term Spatial and Temporal Variations of Aurora Borealis Events in the Period 1700--1905
(1) Instituto de Astrofísica de Canarias, 38200 La Laguna, Spain.
(2) Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Spain
(3) Departamento de Física, Universidad de Extremadura, Avda. Santa Teresa de Jornet 38, 06800, Mérida, Spain.
(4) Departamento de Física, Universidad de Extremadura, 06071 Badajoz, Spain.
PP 013062
Analysis of chemical abundances in planetary nebulae with [WC] central stars. II. Chemical abundances and the abundance discrepancy factor.
(1) IAC, Spain, (2) U. La Laguna, Spain, (3) IA-UNAM, Mexico, (4) PUC, Chile, (5) U. Chile
PP 013061
The Bifurcated Age-Metallicity Relation of Milky Way Globular Clusters and its Implications For the Accretion History of the Galaxy
(1) IAC, (2) Univ. de La Laguna, (3) Univ of Victoria, (4) MPE
PP 013060
Kepler-77b: a very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star
ESA/ESTEC, IAC/ULL, otros
PP 013059
The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey IX: 12CO J=3-2 Observations of NGC 2976 and NGC 3351
Oxford, IAC, otros
PP 013058
A search for near infrared bands of the fullerene cation C$_{60}^+$ in the protoplanetary nebula IRAS 01005+7910
Instituto de Astrof\'\i sica de Canarias, C/ Via L\'actea s/n, 38200 La Laguna, Spain
Departamento de Astrof\'\i sica, Universidad de La Laguna, Spain
PP 013057
ON THE MOLAR EXTINCTION COEFFICIENTS OF THE ELECTRONIC ABSORPTION SPECTRA OF C60 AND C70 FULLERENES RADICAL CATION
[a] CNR–Istituto di Metodologie Chimiche, Area della Ricerca
di Montelibretti, Via Salaria Km 29,300, 00016,
Monterotondo, Scalo, Rome, Italy
[b] Actinium Chemical Research srl, Via Casilina 1626A, 00133
Rome, Italy
[c] Instituto de Astrofisica de Canarias, Via Lactea snc, Tenerife,
Canary Islands, Spain
[d] National Center for Astronomy, KACST, P.O. Box 6086,
Riyad 11442 Saudi Arabia
PP 013056
Massive Clumps in Local Galaxies: Comparisons with High-redshift Clumps
(1) IBM Research Division, USA, (2) Vassar College, USA), (3) IAC and Dep. Astrofisica ULL, Spain)
PP 013055
The long bar as seen by the VVV Survey: II. Star counts
(1) UEFS, Dep. Física, Novo Horizonte, Brazil; (2) UEFS, Obs. Astron. Antares, Jardim Cruzeiro, Brazil; (3) SIM, Univ. Lisbon, Portugal; (4) Lab. Nac. Astrof., Itajubá, Brazil; (5) IAC; (6) ULL; (7) Dep. Fís., Univ. Alicante; (8) Dep. Astron. Astrof., Santiago, Chile; (9) Vatican Obs.; (10) Dep. Física, Univ. Andrés Bello, Santiago, Chile; (11) Obs. Astron. Córdoba, Argentina; (12) Inst. Astron. Teórica Exp., Córdoba, Argentina
PP 013054
Searching for chemical inhomogeneities in Open Clusters: Analysis of the CN and CH Molecular Band Strengths in NGC 2158, NGC 2420, NGC 2682, NGC 7789 and Berkeley 29
1 Instituto de Astrofísica de Canarias, Spain
2 Departamento de Astronomía, Universidad de La Laguna, Spain
PP 013053
The environments of luminous radio galaxies and type-2 quasars
(1) IAC, (2) ULL, (3) University of Sheffield, (4) MPIA, (5) ASTRON, (6) University of Groningen, (7) ORSAY, (8) IFCA, (9) ESA
PP 013052
Hα kinematics of 11 starburst galaxies selected from the Sloan Digital Sky Survey
1Stockholm Observatory, Department of Astronomy, Stockholm University, AlbaNova Center, 106 91 Stockholm, Sweden
1Stockholm University Observatory, Sweden.
2.Oskar Klein Center for Cosmoparticle Physics, University of Stockholm, Sweden
3Instituto de Astrofísica de Canarias,4. Consjeo Superior de Investigaciones Científicas. 5. Departamento de Astrofísica, Universidad de La Laguna, 6. Instituto de Astrofísica de Andalucía
PP 013051
The (galaxy-wide) IMF in giant elliptical galaxies: From top to bottom
(1) IAC, (2) ULL, (3) Mullard Space Science Laboratory, UK, (4) INAF, Italy
PP 013050
X-ray Nuclear Activity in S4G Barred Galaxies: No Link Between Bar Strength and Co-occurrent Supermassive Black Hole Fueling
(1) IAC, (2) ULL, (3) ESO
PP 013049
Low-amplitude rotational modulation rather than pulsations in the CoRoT B-type supergiant HD 46769
(1) Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium
(2) Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
(3) Instituto de Astrofísica de Canarias, 38200, La Laguna, Tenerife, Spain
(4) Departamento de Astrofísica, Universidad de La Laguna, 38205, La Laguna, Tenerife, Spain
PP 013048
Extremely Metal-Poor Galaxies: The H i Content
(1) CentrodeAstrof ́ısicadaUniversidadedoPorto,4150-762,Porto,Portugal,
(2) Max-Planck-Institut fu ̈r Radioastronomie (MPIfR), Auf dem Hu ̈gel 69, 53121 Bonn, Germany,
(3) Instituto de Astrofisica de Canarias,E-38200LaLaguna(Tenerife),Spain
(4) Departamento de Astrofisica, Universidad de LaLaguna,E-38206LaLaguna(Tenerife),Spain
(5) Instituto de Astrof ́ısica de Andalucia,E-18008Granada,Spain
(6) INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040 Monte Porzio Catone, Rome, Italy
(7) Universidad Auto ́noma de Madrid, E-28049 Madrid, Spain
(8) IBM, T. J. Watson Research Center, Yorktown Heights, New York 10598, USA
(9) Vassar College, Department of Physics and Astronomy, Poughkeepsie, New York 12604, USA
PP 013047
Expected number of massive galaxy relics in the present-day Universe
Universidad de Valencia; Instituto de Astrofisica de Canarias; Universidad de La Laguna
PP 013046
The dynamical status of ZwCl 2341.1+0000: a very elongated galaxy structure with a complex radio emission
(1) TNG. Fundación Galileo Galilei, INAF
(2) Osservatorio Astronomico di Trieste (Italy)
(3) Dipartamento di Astronomia. Universita degli Studi di Trieste (Italy)
(4) IAC
(5) DA-ULL
PP 013045
Evidence for quiescent synchrotron emission in the black hole X-ray transient Swift J1357.2-0933
(1)Instituto de Astrofísica de Canarias, (2)Universidad de La Laguna, (3)University of Sheffield, (4)University of Warwick.
PP 013044
Improved search of PCA databases for spectro-polarimetric inversion
(1) HAO, (2) IAC, (3) THEMIS
PP 013043
Dust around R Coronae Borealis stars: II. Infrared emission features in a H-poor environment
(1) IAC-ULL; (2) IIA; (3) McDonald Observatory-UT
PP 013042
The Near Infrared Ca II Triplet as Metallicity Indicator: II Extension to extremely metal-poor metallicity regimes
(1) Instituto de Astrofisica de Canarias, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, Spain
(3) Osservatorio Astronomico di Bologna, Italy
(4) ASI Science Data Center, Italy
PP 013041
Hot bottom burning and s-process nucleosynthesis in massive AGB stars at the beginning of the thermally-pulsing phase
(1) IAC-ULL; (2) INAF-Oss.Rome; (3) Univ. of Vienna; (4) RSAA-ANU; (5) MoCA-Monash Univ.; (6) W.J. McDonald Obs.
PP 013040
Infrared spectroscopy of fullerene C60/anthracene adducts
(1) IAC-ULL; (2) INAF-ACR; (3) CSIC
PP 013039
The mmax-Mecl relation, the IMF and IGIMF: probabilistically sampled functions?
(1) IAC, (2) ULL, (3) AIfA, Bonn
PP 013038
The first spectroscopically identified L dwarf in Praesepe
(1) Instituto de Astrofisica de Canarias, (2) Universidad de La Laguna
PP 013037
CoRoT: harvest of the exoplanet program
(1) LAM, (2) Nice U., (3) LESIA, (4) IAS, (5) IAP, (6) DLR, (7) IAC
PP 013036
On the Origin of Lopsidedness in Galaxies as Determined from the Spitzer Survey of Stellar Structure in Galaxies (S4G)
1 Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA; den- nis.zaritsky@gmail.com
2 Astronomy Division, Department of Physics, P.O. Box 3000, FI-90014 University of Oulu, Finland
3 Finnish Centre of Astronomy with ESO (FINCA), Univer- sity of Turku, V ̈ais ̈al ̈antie 20, FI-21500, Piikkio ̈, Finland
4 Vassar College, Dept. of Physics and Astronomy, Pough- keepsie, NY 12604, USA
5 Aix Marseille Universit ́e, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388, Marseille, France
6 Instituto de Astrof ́ısica de Canarias, V ́ıa L ́acteas 38205 La Laguna, Spain
7 Departamento de Astrof ́ısica, Universidad de La Laguna, 38206, La Laguna, Spain
8 IBM T. J. Watson Research Center, 1101 Kitchawan Road, Yorktown Heights, NY 10598, USA
9 European Southern Observatory, Casilla 19001, Santaigo 19, Chile
10 Departamento de Astrof ́ısica, Universidad Complutense de Madrid, Madrid, Spain
11 MMT Observatory, P.O. Box 210065, Tucson, AZ 85721, USA
12 The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA
13 ESA Fellow, European Space Agency (ESTEC), Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
14 National Radio Astronomy Observatory/ NAASC, 520 Edgemont Road, Charlottesville, VA 22903, USA
15 Spitzer Science Center, 1200 East California Boulevard, Pasadena, CA 91125, USA
16 Max-Planck-Institut fu ̈r Astronomie, K ̈onigstu ̈hl 17 D- 69117, Heidelberg, Germany
17 Observatorio do Valongo, Universidade Federal de Rio de Janeiro, Ladeira Pedro Antnio, 43, Sau ́de CEP 20080-090, Rio de Janeiro-RJ-Brazil
18 California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
19 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
PP 013035
THE IMPACT OF BARS ON DISK BREAKS AS PROBED BY S4G IMAGING
1 National Radio Astronomy Observatory / NAASC, 520 Edgemont Road, Charlottesville, VA 22903
2 DepartamentodeAstrof ́ısica,UniversidadComplutensede Madrid, Madrid 28040, Spain
3 Max-Planck-Institut fu ̈r Astronomie, K ̈onigstuhl 17, 69117 Heidelberg, Germany
4 Aix Marseille Universite, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388, Marseille, France
5 Department of Physical Sciences/Astronomy Division, Univer- sity of Oulu, FIN-90014, Finland
6 Vassar College, Dept. of Physics and Astronomy, Poughkeep- sie, NY 12604
7 IBM Research Division, T.J. Watson Research Center, York- town Hts., NY 10598
8 Instituto de Astrof ́ısica de Canarias, 38205 La Laguna, Spain
9 DepartamentodeAstrof ́ısica,UniversidaddeLaLaguna, 38206 La Laguna, Spain
10 European Southern Observatory, Casilla 19001, Santiago 19, Chile
11 University of Arizona, 933 N. Cherry Ave, Tucson, AZ 85721
12 The Observatories, Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101
13 European Space Agency, ESTEC, Keplerlaan 1, 2200 AG, Noordwijk, the Netherlands
14 Astrophysics, Cosmology and Gravity Centre, Department of Astronomy, University of Cape Town, Private Bag X3, Ronde- bosch 7701, South Africa
15 Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
16 Finnish Centre for Astronomy with ESO (FINCA), University of Turku
17 Observatorio do Valongo, Universidade Federal de Rio de Janeiro, Ladeira Pedro Antonio, 43, Saude CEP 20080-090, Rio de Janeiro - RJ - Brasil
18 Florida Institute of Technology, Melbourne, FL 32901
19 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218
PP 013034
Chemical evolution and the galactic habitable zone of M31 (the Andromeda Galaxy)
(1) IA-UNAM, Mexico, (2) IAC, Spain, (3) ULL, Spain, (4) Kapteyn Instituut, Nederlands
PP 013033
Spatial dependence of the Star Formation History in the Central Regions of the Fornax Dwarf Spheroidal Galaxy
(1) IAC, (2) University of La Laguna, (3) INAF--Osservatorio Astronomico di Teramo, (4) ESO Chile.
PP 013032
Stability Toward High Energy Radiation of Non Proteinogenic Amino Acids: Implications for the Origins of Life
1
Actinium Chemical Research srl, Via Casilina 1626A, 00133 Rome, Italy
E
-
Mail
:
franco.cataldo@fastwebnet.it
2
Osservatorio Astrofisico di Catania, Via S.
Sofia 78, 95123 Catania, Italy
;
3
National Center for Astronomy, KACST, P.O. Box 6086, Riyad 11442 Saudi Arabia
4
Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300, Monterotondo Stazione 00016,
Rome, Italy
5
Instituto de Astrofisica de C
anarias, Via Lactea s/n, 38200 La Laguna, Tenerife, Spain
Universidad de La Laguna, Spain
PP 013031
Arqueología del cielo. Orientaciones astronómicas en edificios protohistóricos del sur de la Península Ibérica
(1) IAC, (2) Dpto. de Prehistoria y Arqueología, Universidad de Sevilla
PP 013030
NGC 2579 and the carbon and oxygen abundance gradients beyond the solar circle
(1) IAC, (2) Departamento de Astrofísica, ULL, (3) Intituto de Astronomía, UNAM, (4) Universidade Federal de Santa Maria, (5) LUTH, Observatoire de Paris-Meudon, (6) Pontificia Universidad Católica de Chile,
(7) Departamento de Física, IPN
PP 013029
Determination of Coronal Transverse Density Structuring from Propagating MHD Waves in the Solar Atmosphere
(1) Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38205 La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain, (3) School of Mathematics and Statistics, University of St. Andrews, St. Andrews, KY16 9SS, UK
PP 013028
Coronal loop physical parameters from the analysis of multiple observed transverse oscillations
IAC
PP 013027
Constraints on the Sunyaev-Zeldovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
1 Instituto de Astrofísica de Canarias
2 Departamento de Astrofísica, Universidad de La Laguna
3 Leibniz Institut für Astrophysik, Potsdam
4 Física Teórica, Universidad de Salamanca
PP 013026
Solid state radiolysis of non-proteinaceous amino acids in vacuum: astrochemical implications
F. Cataldo
a Istituto Nazionale di Astrofisica, Osservatorio Astrofisica di Catania,Italy
b Chemical Research, Rome,Italy
G. Angelini
c Istituto di Metodologie Chimiche, CNR, Rome, Italy
Y. Hafez
d National Center for Astronomy, Saudi Arabia
S. Iglesias-Groth
e Instituto de Astrofisica de AStrofísica de Canarias
f Universidad de la laguna
PP 013024
On the Radical Anion Spectra of Fullerenes C60 and C70
a Instituto Nazionale di Astrofisica, Osservatorio Astrofisico di
Catania, Catania, Italy
b Actinium Chemical Research, Rome, Italy
c Instituto de Astrofísica de Canarias (IAC),Universidad de La laguna, Tenerife, Spain
d CSIC, Madrid, Spain
PP 013023
A 2 hour periodic variation in the low mass a9a X-ray binary Ser X-1
1) IAC 2) ULL 3) University of Southampton 4) University of Capetown 5) University of Warwick
PP 013022
The SUMO project I. A survey of multiple populations in globular clusters
(1)Instituto de Astrofisica de Canarias,
(2)Departamento de Astrofisica, Universidad de La Laguna,
(3)Research School of Astronomy & Astrophysics, ANU,
(4)Dominion Astrophysical Observatory,
(5)Max-Planck-Institut fur Astrophysik Karl-Schwarzschild-Str,
(6)INAF-Osservatorio Astronomico di Teramo,
(7)Astrophysics Research Institute, Liverpool John Moores University,
(8)Department of Physics and Astronomy, Aarhus University,
(9)Dipartimento di Fisica e Astronomia, Universita' di Padova,
(10)INAF-Osservatorio Astronomico di Padova,
(11)Zentrum fur Astronomie der Universitat Heidelberg.
PP 013021
Kinematics of Arp 270: gas flows, nuclear activity, and two regimes of star formation
(1) IAC, (2) Department of Astrophysics, University of La Laguna, (3) CSIC, (4)
IAA, (5) XMM-Newton Science Operations Centre, (6) UNAM
PP 013020
The filling factor - radius relation for 58 H II regions across the disk of NGC 6946
1. IAC 2. Departamento de Astrofísica ULL, 3. CSIC, 4. Dto. Ing. Elettrónica, U. Roma Tor Vergata %. Instituto de Astrofísica de Andalucía.
PP 013019
Peaks in the CMBR power spectrum. II. Physical interpretation for any cosmological scenario
IAC, ULL
PP 013018
The VLT-FLAMES Tarantula Survey. IX. The interstellar medium seen through Diffuse Interstellar Bands and neutral sodium
Varias (VFTS Consortium)
PP 013017
The VLT-FLAMES Tarantula Survey X: Evidence for a bimodal distribution of rotational velocities for the single early B-type stars
Varias (VFTS consortium)
PP 013016
No temperature fluctuations in the giant HII region H 1013
OPM, UNAM, IAC, IfA, ObsGe, U. Leiden
PP 013014
Statistical Studies of HII Regions in the Nearby Galaxies. 1. Spitzer NIR luminosities and temperatures, compared with Halpha luminosities, of selecte4d HII regions in M100
1 43 Tamar Way, Didcot, OX11 7QH, United Kingdom
e-mail: sjchan2012@gmail.com
2 Instututo de Astrofisica de Canarias, 38205 La Laguna, Spain
e-mail: jeb@iac.es
3 CSIC, 28006 Madrid, Spain
4 Department of Astrophysics, University of La Laguna, E-38200 La Laguna, Tenerife, Spain
PP 013013
Estimations of the magnetic field strength in the torus of AGN using near-infrared polarimetry
(1)UTSA, (2)UF, (3)Univ. of Hertfordshire, (4)UKY, (5)Gemini Observatory South, (6)Gemini Observatory North, (7)IAC, (8)ULL, (9)IFCA, (10)Univ. of Minnesota, (11)FIT
PP 013012
Searching for the signatures of terrestrial planets in F-, G-type main-sequence stars
(1) Instituto de Astrofísica de Canarias,
(2) Depto. Astrofísica, Universidad de La Laguna,
(3) Centro de Astrofísica, Universidade do Porto,
(4) Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto,
(5) Observatoire Astronomique de l'Université de Genève
PP 013011
Galactic kinematics of planetary nebulae with [WC] central star
(1) Instituto de Astronomía, UNAM, Mexico
(2) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
(3) Departamento de Astrofísica. Universidad de La Laguna, tenerife, Spain
PP 013009
Planck intermediate results. VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters
IAC and others
PP 013008
Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
IAC and others
PP 013007
Local tadpole galaxies: dynamics and metallicity
(1) Instituto de Astrofisica de Canarias, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain
(3) Department of Physics and Astronomy, Vassar College, NY, USA
(4) IBM Research Division, Watson Research Center, NY, USA
PP 013006
Bayesian Analysis of Multiple Harmonic Oscillations in the Solar Corona
(1) Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 013005
The changing nebula around the hot R Coronae Borealis star DY Centauri
(1) IIA; (2) McDonald Observatory-UT; (3) IAC; (4) ULL; (5) CSIC
PP 013004
The puzzling merging cluster Abell 1914: new insights from the kinematics of member galaxies
(1) IAC
(2) ULL
(3) Osservatorio Astronomico di Trieste, Italy
(4) Universita degli Studi di Trieste, Italy
(5) Fundacion Galileo Galilei - INAF, Spain
PP 013003
KIC 10449976: discovery of an extreme helium subdwarf in the Kepler field
(1) Armagh Observatory, College Hill, Armagh BT61 9DG, UK (2) Instituto de Astrofísica de Canarias, La Laguna E-3200, Tenerife, Spain (3) Departamento de Astrofísica, Universidad de La Laguna, La Laguna E-38205, Tenerife, Spain (4) Department of Physics, University of Warwick, Coventry CV4 7AL, UK (5) NASA Ames Research Center, M/S 244-40, Moffett Field, CA 94035, USA (6) Bay Area Environmental Research Institute, Inc., 560 Third St. West, Sonoma, CA 95476, USA (7) Isaac Newton Group of Telescopes, Apartado de Correos 321, E-38700 Santa Cruz de la Palma, Canary Islands, Spain (8) Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK (9) Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäl äntie 20, FI-21500 PIIKKIÖ, Finland
PP 013002
Diffuse interstellar bands in fullerene planetary nebulae: the fullerenes - diffuse interstellar bands connection
(1) IAC; (2) ULL
PP 013001
Wave Leakage and Resonant Absorption in a Loop Embedded in a Coronal Arcade
(1) Departament de Fisica, Universitat de les Illes Balears. E- 07122 Palma de Mallorca, Spain
(2) Instituto de Astrofisica de Canarias, Via Lactea s/n. E- 38205 La Laguna, Spain
(3) Departament de Astrofisica, Universidad de La Laguna. E- 38205 La Laguna, Spain