Preprints in 2009
PP 09070
Planck pre-launch status: Design and description of the Low Frequency Instrument
1 Universit`a degli Studi di Milano, Dipartimento di Fisica, via Celoria 16, 20133 Milano, Italy (e-mail: marco.bersanelli@unimi.it) 2 INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, via Bassini 15, 20133 Milano, Italy 3 INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, via P. Gobetti, 101, I40129 Bologna, Italy 4 Universidad de Cantabria, Departamento de Ingenieria de Comunicaciones, av. de Los Castros s/n, 39005 Santander, Spain. 5 Thales Alenia Space Italia S.p.A., S.S. Padana Superiore 290, 20090 Vimodrone, Milano, Italy 6 SISSA/ISAS, Astrophysics Sector, Via Beirut 4, 34014 Trieste, Italy 7 CESR, Centre dEtude Spatiale des Rayonnements, 9, av du Colonel Roche, BP 44346 31028 Toulouse Cedex 4, France 8 Instituto de Fisica de Cantabria, CSIC, Universidad de Cantabria, av. de los Castros s/n, 39005 Santander, Spain 9 Jodrell Bank Centre for Astrophysics, Alan Turing Building, The University of Manchester, Manchester, M13 9PL, UK 10 Herschel/Planck Project, Scientific Projects Dpt of ESA, Keplerlaan 1, 2200 AG, Noordwijk, The Netherlands 11 Istituto di Fisica del Plasma, CNR, via Cozzi 53, 20125 Milano, Italy 12 ASI, Agenzia Spaziale Italiana, viale Liegi, 26, 00198 Roma, Italy 13 Dipartimento di Fisica, Universit`a degli Studi di Roma Tor Vergata, via della Ricerca Scientifica 1, 00133 Roma, Italy 14 INAF Osservatorio Astronomico di Padova, Vicolo dell Osservatorio 5, 35122 Padova, Italy 15 INAF Osservatorio Astronomico di Trieste, via Tiepolo, 11, I-34143 Trieste, Italy 16 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 17 Instituto de Astrofisica de Canarias, C/ Via Lactea s/n, 38200, La Laguna, Tenerife, Spain 18 Dipartimento di Fisica, Universit`a degli Studi di Trieste, via A. Valerio 2, 34127 Trieste, Italy
PP 09069
The SAURON project - XV. Modes of star formation in early-type galaxies and the evolution of the red sequence
(1) Berkeley (2) IAC (3) ESA/ESTEC (4) IAS (5) ESO-Garching (6) STRW-Leiden (7) CfA-Hatfield (8) CRAL-Lyon (9) Univ. of Maryland (10) Oxford Univ. (11) Swinburne (12) Gemini-Hawaii (13) RUG-Groningen (14) Univ. of Austin Texas
PP 09068
VSA Observations of the Anomalous Microwave Emission in the Perseus Region
(1) Jodrell Bank Centre for Astrophysics, University of Manchester, UK
(2) Instituto de Astrofisica de Canarias, Spain
(3) UNINOVA/CA3, Caparica, Portugal
(4) Cavendish Laboratory, Cambridge, UK
(5) University de la Laguna, Spain
(6) Kavli Insitute for Cosmology, Cambridge
(7) Consejo Superior de Investigaciones Cientificas, Spain
PP 09067
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-yr data: II – Flux density variability
(1) Astrophysics Group, Cavendish Laboratory, University of Cambridge
(2) Jodrell Bank Centre for Astrophysics, University of Manchester
(3) Instituto de Astrofísica de Canarias, Universidad de La Laguna
(4) Kavli Institute for Cosmology Cambridge
PP 09066
Follow-up observations at 16 and 33GHz of extragalactic sources from WMAP 3-yr data: I - Spectral properties
(1) Astrophysics Group, Cavendish Laboratory, University of Cambridge
(2) Jodrell Bank Centre for Astrophysics, University of Manchester
(3) Instituto de Astrofísica de Canarias, Universidad de La Laguna
(4) Kavli Institute for Cosmology Cambridge
PP 09064
The chemical composition of TS01, the most oxygen-deficient planetary nebula. AGB nucleosynthesis in a metal-poor binary star
(1) LUTH, Observatoire de Paris
(2) IAC
(3) ULL
PP 09063
The JCMT Nearby Galaxies Legacy Survey III: Comparisons of cold dust, polycyclic aromatic hydrocarbons, molecular gas, and atomic gas in NGC 2403
Muchas, incl. IAC & ULL
PP 09062
On the Magnetic Field of off-limb Spicules
(1) HAO - National Center for Atmospheric Research
(2) IAC - Instituto de Astrofísica de Canarias
(3) Departamento de Astrofísica (Universidad de La Laguna)
(4) CSIC - Consejo Superior de Investigaciones Científicas
PP 09061
155-day Periodicity in Solar Cycles 3 and 4
(1) Departamento de Física Aplicada, Escuela Politécnica, Universidad de Extremadura, Cáceres, Spain.
(2) CGUL-IDL, Universidade de Lisboa, Lisbon, Portugal.
(3) Departamento de Eng. Civil da Universidade Lusófona, Lisbon, Portugal.
(4) Instituto de Astrofísica de Canarias, 38200 La Laguna, Spain.
(5) Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Spain
(6) Departamento de Física, Universidad de Extremadura, Badajoz, Spain.
PP 09060
The chemical composition of the Orion star forming region: I. Homogeneity of O and Si abundances in B-type stars
IAC, ULL
PP 09059
On the curvature of dust lanes in galactic bars
(1) Instituto de Astrofísica de Canarias, E-38200 La
Laguna, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
(3) Consejo Superior de Investigaciones Científicas, Spain
PP 09057
Resolved Dust Emission in a Quasar at z = 3.65
(1)Physics Department, Imperial College, Prince Consort Road, London SW7 2AZ, UK
(2)Submillimetre Array, Hilo, HI, USA
(3)Astronomy Centre, University of Sussex, Brighton, BN1 9QH, UK
(4)European Southern Observatory, Garching, Munich, Germany
(5)IAC, Tenerife, Spain
(6)IPAC, Caltech, Pasadena, CA, USA
(7)Spitzer Science Centre, Caltech, Pasadena, CA, USA
(8)Universita di Padova, Padova, Italy
(9)Harvard-Smithsonian Centre for Astrophysics, Cambridge, MA, USA
(10)UCSD, San Diego, CA, USA
PP 09056
Intracluster light in the Virgo Cluster: Large scale distribution
(1)Instituto de Astrofísica de Canarias,
(2)European Southern Observatory,
(3)INAF, Osservatorio Astronomico di Pino Torinese
(4)Max-Planck-Institut Institut für Extraterrestrische Physik
(5)Department of Astronomy and Research Center for the Early Universe, School of Science, University of Tokyo
(6)Institute for Cosmic Ray Research, University of Tokyo
(7)Research School of Astronomy and Astrophysics, Mount Stromlo Observatory
PP 09055
HD 172189: another step in furnishing one of the best laboratories known for asteroseismic studies
1 Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain.
2 Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain.
3 Laboratoire AIM, CEA/DSM-CNRS-Université Paris, Diderot; CEA,IRFU, SAp, centre de Saclay, F-91191, Gif-sur-Yvette, France.
4 Instituto de Astrofísica de Andalucía (CSIC), Camino bajo de Huétor 50, 18080 Granada, Spain.
5 Astronomical Institute, Wrocław University, Kopernika 11, 52-622 Wrocław, Poland.
6 Instituut voor Sterrenkunde, Celestijnenlaan, 200D, 3001 Leuven, Belgium.
7 Laboratoire d’Astrophysique de Toulouse-Tarbes, Université de Toulouse, CNRS 31400 - Toulouse, France.
8 Universidad de Vigo, Departamento de Física Aplicada, Campus Lagoas-Marcosende, 36310-Vigo, Spain.
9 Mercator Telescope, Observatorio del Roque de los Muchachos, Apartado de Correos 474, 38700 Santa Cruz de La Palma, Spain.
10 INAF-OABrera, Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate, Italy.
11 Instituto de Astronomía, Universidad Nacional Autónoma de Mexico, Apdo. Postal 70-264, 04510 Mexico D.F., Mexico.
12 UNS, CNRS, OCA, Campus Valrose, UMR 6525 H. Fizeau, F-06108 Nice Cedex 2, France.
13 UPMC Univ. Paris 06, UMR 7585, Laboratoire de Physique Nucléaire et des Hautes Energies (LPNHE), F-75005 Paris, France.
14 Astronomical Institute, Academy of Sciences, Bocni II 1401, CZ - 141 31 Praha 4, Czech Republic.
15 INAF Catania Astrophysical Observatory, via S. Sofia, 78-95123, Catania, Italy.
PP 09054
The Physical Orgin and the Diagnostic Potential of the Scattering Polarization in the Lithium Resonance Doublet at 6708 \AA.
(1) University of Florence
(2) Instituto de Astrofisica de Canarias
(3) Consejo Superior de Investigaciones Cientificas
PP 09053
Compressive Sensing for Spectroscopy and Polarimetry
(1) Instituto de Astrofisica de Canarias
(2) Departamento de Astrofisica, Universidad de La Laguna
(3) THEMIS
PP 09052
Rb-rich Asymptotic Giant Branch stars in the Magellanic Clouds
(1) IAC, (2) CSIC, (3) W. J. McDonald Observatory, (4) GRAAL-Universite Montpellier 2, (5) Herschel Science Centre, ESAC-ESA, (6) INAF-Osservatorio Astronomico di Roma, (7) CSPA-Monash University, (8) RSAA-Mt Stromlo Observatory, (9) University of Utrecht
PP 09051
On the origin of reverse polarity patches found by Hinode in sunspot penumbrae
((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain,
(2) Departamento de Astrofisica, Universidad de La Laguna,
(3) Kwasan and Hida Observatories, Kyoto University, Kyoto, Japan)
PP 09050
Pattern Speeds of Bars and Spiral Arms from Halpha Velocity Fields
(1) IAC, (2) University of Stockholm, (3) CSIC (4) U. La Laguna.(5) U. Montreal.
PP 09049
Transit timing analysis of the exoplanets TrES-1 and TrES-2
(1) IAC, (2) ULL, (3) Laboratoire d'Astrophysique de Marseille, (4) Observatoire de Genève, Université de Genève
PP 09048
The Sunyaev-Zeldovich effect in superclusters of galaxies using gasdynamical simulations: the case of Corona Borealis
(1) IAC, (2) Departamento de Astrofísica (ULL), (3) Department of
Physics, University di Roma "La Sapienza", (4)CSIC, (5) Grupo de Astrofísica, UAM, (6) Astrophysikalisches Institut Potsdam
PP 09047
Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
(1) Centro Studi e Ricerche Enrico Fermi, Rome, Italy, (2) Istituto de Sistemi Complessi CNR, Rome, Italy, (3) Institute of Astronomy, St. Petersburg State Univ., Russia, (4) IAC
PP 09046
Are Dry Mergers Dry, Moist, or Wet?
(1) Jeremiah Horrocks Insitute for Astrophisics & Supercomputing, UCLan, Preston, PR1 2HE, UK
(2) Instituto de Astrofisica de Canarias, c/Via Lactea s/n, 38205, La Laguna, Tenerife, Spain.
(3) Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
(4) Mullard Space Science Laboratory, Holmbury St Mary, RH5 6NT, UK
(5) Departamento de Astrofisica y CC de la Atmosfera, Universidad Complutense de Madrid, Av Complutense s/n, 28040, Madrid, Spain
PP 09045
Ground-based photometry of space-based transit detections: Photometric follow-up of the CoRoT mission
(1) IAC, (2) Obs. Gèneva, (3) U. Liège, (4) Tel Aviv Univ., (5) LESIA Paris, (6) Tautenburg
PP 09044
Rate and nature of false positives in the CoRoT exoplanet search
(1) IAC, (2) U. Exeter, (3) LAM Marseilla, (4) LESIA Paris
PP 09043
The onset of solar cycle 24: What global acoustic modes are telling us
(1) IAC, (2) CEA, Centre de Saclay, France
PP 09042
Study of star-forming galaxies in SDSS up to redshift 0.4 I. Metallicity evolution
Instituto de Astrofísica de Canarias, 38200 La Laguna, Spain
Departamento de Astrofísica, Universidad de la Laguna, Spain
Departamento de Física, Escuela Superior de Física y Matemática, IPN, México D.F., México
Herschel Science Center, INSA/ESAC, Madrid, Spain
PP 09041
AINUR: Atlas of Images of NUclear Rings
(1) IAC, (2) CSIC, (3) University of Oulu, (4) University of Alabama
PP 09040
Unveiling the nature of M94's (NGC4736) outer region: a panchromatic perspective
(1) IAC
(2) Institute of Astronomy, University of Cambridge
(3) Blackbird Observatory, New Mexico, USA
(4) Cardiff University, School of Physics \& Astronomy
PP 09039
The Infrared Nuclear Emission of Seyfert Galaxies on Parsec Scales: Testing the Clumpy Torus models
(1)IAC (2)Department of Physics and Astronomy, University of Kentucky
(3)Instituto de Estructura de la Materia, CSIC, (4)Gemini South Observatory
(5)Astronomy Department, University of Florida, (6)Gemini Observatory, Northern Operations Centre
PP 09037
Multiline Zeeman Signatures Through Line Addition
(1) LESIA, (2) LERMA, (3) IAC, (4) Institute for Astronomy, U. of Vienna, (5) THEMIS, (6) INAF-Catania
PP 09036
Earth’s transmission spectrum from lunar eclipse observations
Instituto de Astrofisica de Canarias
PP 09035
A STELLAR MODEL-FITTING PIPELINE FOR ASTEROSEISMIC DATA FROM THE KEPLER MISSION
1 High Altitude Observatory and Scientific Computing Division, NCAR, P.O. Box 3000, Boulder, CO 80307, USA
2 Instituto de Astrofísica de Canarias, 38205, La Laguna, Tenerife, Spain
3 Newkirk Graduate Fellow, High Altitude Observatory, NCAR, P.O. Box 3000, Boulder, CO 80307, USA
4 Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
5 Affiliate Scientist, High Altitude Observatory, NCAR, P.O. Box 3000, Boulder, CO 80307, USA
PP 09034
Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission
1 Sydney Institute for Astronomy (SIfA), School of
Physics, University of Sydney, NSW 2006, Australia;
stello@physics.usyd.edu.au.
2 Danish AsteroSeismology Centre (DASC), Department of
Physics and Astronomy, Aarhus University, 8000 Aarhus C,
Denmark
3 School of Physics and Astronomy, University of Birmingham,
Edgbaston, Birmingham, B15 2TT, UK
4 Instituto de Astrof ́ ısica de Canarias, E-38200, La Laguna,
Tenerife, Spain
5 Instituto de Astrof ́ ısica de Andaluc ́ ıa, CSIC, CP3004,
Granada, Spain
6 Centro de Astrof ́ ısica da Universidade do Porto, Rua das
Estrelas, 4150-762 Porto, Portugal
7 Departamento de Matem ́tica Aplicada, Faculdade de Ciˆncias
a e
da Universidade do Porto, Portugal
8 Institut d’ Astrophysique Spatiale (IAS), UMR8617, Batiment
121, F-91405, Orsay Cedex, France
9 Max-Planck-Institut f ̈ r Astrophysik, Karl-Schwarzschild-Str.
u
1, Postfach 1317, 85741, Garching, Germany
10 Laboratoire d RAstrophysique de Toulouse-Tarbes, Universit
de Toulouse, CNRS, 14 avenue Edouard Belin, F-31400 Toulouse,
France
11 Faculty of Arts, Computing, Engineering and Sciences,
Sheffield Hallam University, Sheffield S1 1WB, UK
12 Laboratoire AIM, CEA/DSM-CNRS-Universit ́ Paris e
Diderot; CEA, IRFU, SAp, centre de Saclay, F-91191, Gif-sur-
Yvette, France
13 Institute of Astronomy, University of Vienna, A-1180 Vienna,
Austria
14 Institute of Astronomy, University of Cambridge, Cambridge
CB3 0HA, UK
15 Departamento de Astrof ́ ısica, Universidad de La Laguna, La
Laguna, 38206, Tenerife, Spain
16 National Solar Observatory, 950 North Cherry Avenue,
Tucson, AZ 85719, USA
PP 09033
Stellar populations in the centres of brightest cluster galaxies
(1) JeremiahHorrocksInstituteforAstrophysicsandSupercomputing, Universityof Central Lancashire, Preston, PR12HE, UK
(2) Instituto de Astrofisica de Canarias, c/via Lactea s/n, 38204, La Laguna, Tenerife, Spain
(3) Oxford Astrophysics, Department of Physics, University of Oxford, OX1 3RH, UK
(4) PhysicsDepartment, Universityof theWesternCape, CapeTown7535, SouthAfrica
PP 09032
The Origin of the Light Distribution in Spiral Galaxies
(1) Instituto de Astrofisica de Canarias, c/Via Lactea s/n, E38205, La Laguna, Tenerife, Spain
(2) 1Jeremiah Horrocks Institute for Astrophysics and Supercomputing,Preston, PR1 2HE, UK
PP 09031
Magnetic field strength of active region filaments
(1) IAC, (2) HAO (NCAR), (3) Institute of Space and Astronautical Science (JAXA)
PP 09030
Internal dynamics of the galaxy cluster Abell 959
(1) Fundacion Galileo Galilei - INAF, Rambla Jose Ana Fernandez Perez 7,
E-38712 Brena Baja (La Palma), Canary Islands, Spain
(2) Dipartimento di Astronomia of the Universita degli Studi
di Trieste, via Tiepolo 11, I-34143 Trieste, Italy
(3) IAC
(4) INAF - Osservatorio Astronomico di Trieste, via Tiepolo 11,
I-34143 Trieste, Italy
PP 09029
Internal dynamics of Abell 1240: a galaxy cluster with symmetric double radio relics
(1) IAC
(2) Dipartimento di Astronomia of the Universit\`a degli Studi di Trieste, via Tiepolo 11, I-34143 Trieste, Italy
(3) INAF - Osservatorio Astronomico di Trieste, via Tiepolo 11, I-34143 Trieste, Italy
(4) Fundaci\'on Galileo Galilei - INAF, Rambla Jose Ana Fernandez Perez 7,
E-38712 Brena Baja (La Palma), Canary Islands, Spain
(5) Max-Planck-Institut fur Sonnensystemforschung, Max-Planck-Str. 2, G-37191 Katlenburg-Lindau, Germany
PP 09027
The H alpha Galaxy Survey. VIII. Close companions and interactions, and the definition of starbursts
IAC, LJMU
PP 09026
The H alpha Galaxy Survey VII. The spatial distribution of star formation within disks and bulges
LJMU, LJMU, IAC
PP 09025
Do Bars Drive Spiral Density Waves?
Alabama, IAC, IBM, Oulu, Oulu, Vassar, INAOE, Witwatersrand
PP 09024
The contribution of the kinematic Sunyaev-Zel'dovich Effect from the Warm Hot Intergalactic Medium to the Five-Year WMAP Data
(1) Instituto de Astrofisica de Canarias, Spain
(2) Cavendish Laboratory, University of Cambridge, UK
(3) Fisica Teórica, Universidad de Salamanca, Spain
(4) Astrophysikalisches Institut Potsdam, Germany
PP 09023
The Young Stellar Population of IC1613. I. A New Catalogue of OB associations.
(1) Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38200 La Laguna, Tenerife, Spain.
(2) Dpto. de Astrofisica, Universidad de La Laguna, Avda. Astrofisico Francisco Sanchez s/n, E-38071 La Laguna, Tenerife, Spain.
(3) Current address: Instituto de Astrofisica de Andalucia, CSIC, Apdo. 3004, E-18080, Granada, Spain
(4) Instituto de Astronomia y Meteorologia, Universidad de Guadalajara, Av. Vallarta No. 2602, Guadalajara, Jalisco, C.P. 44130, Mexico
PP 09022
The stellar population of the star forming region G61.48+0.09
(1) IAC, (2) Departamento de Astrofisica Molecular e Infrarroja, IEM, CSIC, Madrid, Spain, (3) Rochester Institute of Technology, Rochester, NY, USA
PP 09021
Search for blue compact dwarf galaxies during quiescence II: metallicities of gas and stars, ages, and star-formation rates
IAC
PP 09020
The spatial distribution of galaxies within the CMB cold spot in the Corona Borealis supercluster
Instituto de Astrofísica de Canarias
Consejo Superior de Investigaciones Científicas
PP 09019
Mg and TiO spectral features at the near-IR: Spectrophotometric index definitions and empirical calibrations
(1) IAC, (2) Universidad Complutense de Madrid
PP 09017
Evidence for the disky origin of luminous Virgo dwarf ellipticals from the kinematics of their globular cluster systems
(1) IAC
(2) Harvard-Smithsonian Center for Astrophysics
(3) UCO/Lick Observatory, University of California, Santa Cruz
PP 09016
The Lunar Terrestrial Observatory: Observing the Earth using photometers on the Moon's surface
Instituto de Astrofisica de Canarias
New Jersey Institute of Technology
PP 09015
BayesCLUMPY: Bayesian Inference with Clumpy Dusty Torus Models
Instituto de Astrofísica de Canarias
PP 09014
A Topology for the Penumbral Magnetic Fields
Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
PP 09013
Measurement of low signal-to-noise-ratio solar p modes in spatially-resolved helioseismic data
(1) National Solar Observatory, (2) Instituto de Astrofísica de Canarias, (3) Institut d'Astrophysique Spatiale
PP 09012
The Chemical Evolution of Globular Clusters I. Reactive Elements and Non-Metals
(1) Jeremiah Horrocks Institute for Astrophysics & Supercomputing, University of Central Lancashire, Preston, PR1 2HE, UK
(2) Research School of Astronomy & Astrophysics, Mt Stromlo Observatory, Weston Creek ACT 2611, Australia
(3)Instituto de Astrofísica de Canarias; c/Vía Láctea s/n, E38205, La Laguna (Tenerife), Spain.
PP 09011
The mixed chemistry phenomenon in Galactic Bulge Planetary Nebulae
(1): European Space Astronomy Centre, INSA S.A. P.O. Box 78, E-28080 Madrid, Spain ; (2): Instituto de Astrofisica de Canarias, C/ Via Lactea s/n, 38200 La Laguna, Spain; (3): Herschel Science Centre. European Space Astronomy Centre, Research and Scientific Support Department of ESA, Villafranca del Castillo, P.O. Box 78, E-28080 Madrid, Spain; (4): N. Copernicus Astronomical Center, Rabianska 8, 87-100 Torun, Poland; (5) Department of Physics. University of Maryland, College Park, MD 20742-4111, USA
PP 09010
Properties of the ionized gas in HH202. II: Results from echelle spectrophotometry with UVES
^1Instituto de Astrof\'\i sica de Canarias, E-38200 La Laguna, Tenerife, Spain
^2Instituto de Astronomí a, UNAM, Apdo. Postal 70-264, 04510 México D.F., Mexico
^3Instituto de Astrofísica de Andalucía (CSIC), Apdo. Correos 3004, E-18080 Granada, Spain
^4Deparment of Physics, Virginia Polytechnic and State University, Blacksburg, VA 24061, USA
^5Instituto Nacional de Astrofísica, Óptica y Electrónica INAOE, Apdo. Postal 51 y 216, 7200 Puebla, Pue., Mexico
PP 09009
Properties of the ionized gas in HH202. I: Results from integral field spectroscopy with PMAS
^1 Instituto de Astrof\'\i sica de Canarias, E-38200 La Laguna, Tenerife, Spain
^2 Instituto de Astronom\'\i a, UNAM, Apdo. Postal 70-264, 04510 M\'exico D.F., Mexico
^3 Instituto de Astrof\'\i sica de Andaluc\'\i a (CSIC), Apdo. Correos 3004, E-18080 Granada, Spain
PP 09008
CNO abundances of HdC and RCB stars: a view of the nucleosynthesis in a white dwarf merger
(1): Instituto de Astrofisica de Canarias (IAC)
(2): National Optical Astronomy Observatory (NOAO)
(3): W. J. McDonald Observatory. The University of Texas at Austin
(4): Department of Physics and Astronomy, Uppsala University
PP 09007
Aligned Electromagnetic Excitations of a Black Hole and their Impact on its Quantum Horizon
a Gravity Research Group, NSI, Russian Academy of Sciences,Russia
b Instituto de Ciencias del Espacio (CSIC) & Institut d’Estudis Espacials de Catalunya (IEEC/CSIC), Spain
c Instituto de Astrofísica de Canarias, Spain
d Dipartimento di Matematica del Politecnico di Milano, Italy
PP 09006
Robust determination of the major merger fraction at z = 0.6 in Groth Strip
(1)IAC, (2)ESO-Garching, (3)ULL, (4)IAA, (5)UCM, (6)MPE, (7)UF
PP 09004
Near-Infrared Spectroscopy of Seyfert Galaxies. Nuclear Activity and Stellar Population
IAC
PP 09003
The ACS Survey of Galactic Globular Clusters. VII. Relative Ages
(1) Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38200 La Laguna, Spain, (2) Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611, (3) University of La Laguna, Spain, (4) Dipartimento di Astronomia, Universita di Padova, 35122 Padova, Italy, (5) Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, (6) University of Texas, McDonald Observatory, 1 University Station, C1402, Austin TX, 78712, (7) Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD 21218, (8) Dept. of Astronomy, Univ. of Washington, Box 351580, Seattle, WA 98195-1580, (9) Dept. of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325
PP 09002
The JCMT Nearby Galaxies Legacy Survey I. Star Forming Molecular Gas in Virgo Cluster Spiral Galaxies
McMaster and various others
PP 09001
Bars, ovals and lenses in early-type disk galaxies: probes of galaxy evolution
Oulu, Oulu, Alabama, IAC