Preprints in 2010
PP 010087
Properties of the HII regions of M51 and NGC 4449 from Halpha images with ACS on HST.
1.Universidad Nacional Autónoma de México, Instituto de Astronomía, Ensenada, B.C.México. 2. Instituto de Astrofísica de Canarias. 3.Consejo Superior de Investigaciones Científicas, España. 4. Facultad de Física, Universidad de La Laguna 5. Universidad Nacional Autónoma de México, Centro de Radioastronomía y Astrofísica, Morelia, México.
PP 010086
Lucky Imaging Adaptive Optics of the browndwarf binary GJ569Bab
(1) IAC, (2) Departamento de Astrofísica Universidad de La Lagun, (3) CSIC, (4) Laboratoire de Physique Subatomique et Cosmologie-Grenoble, (5) Universidad Politécnica de Cartagena-Murcia, (6) Max-Planck-Institut für Sonnensystemforschung-Katlenburg-Lindau, Germany
PP 010084
INFRARED SPECTROSCOPY AND INTEGRATED MOLAR ABSORPTIVITY OF C60 AND C70 FULLERENES AT EXTREME TEMPERATURES
1Instituto de Astrofísica de Canarias, Via Lactea s/n, E-38200, La Laguna,
Tenerife, Spain
2Istituto Nazionale di Astrofisica – Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy
3Actinium Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy
4 Consejo Superior de Investigaciones Científicas, Spain
5 Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 010083
On the magnitude difference between the main sequence turn off and the red giant branch bump in Galactic globular clusters
(1) INAF - Osservatorio Astronomico di Teramo, (2) Centro de Estudios de Fisica del Cosmos de Aragon (CEFCA), (3) Departamento de Astrofisica, Universidad Complutense de Madrid, (4) Astrophysics Research Institute, Liverpool John Moores University, (5) Departamento de Astrofísica, Universidad de La Laguna, (6) IAC
PP 010082
Photospheric Hanle diagnostic of weak magnetic dipoles in stars
(1) THEMIS
(2) IAC
(3) Departamento de Física, Ingenieria de Sistemas y Teoría de
la Señal, Universidad de Alicante
PP 010081
The most recent burst of Star Formation in the Massive Elliptical Galaxy NGC 1052
((1) Instituto de Astrofísica de Canarias, (2) Departamento de Astrofísica, Universidad de La Laguna, (3) Laboratoire d'Astrophysique de Marseille)
PP 010080
The JCMT Nearby Galaxies Legacy Survey VI: The distribution of gas and star formation in M81
IAC, ULL, others
PP 010078
Modeling Star counts in the Monoceros stream and the Galactic anti-centre
1- IAC, 2- ULL, 3- ESO, Garching, Germany
PP 010077
HerMES : SPIRE detection of high redshift massive compact galaxies in GOODS-N field
1Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain
2Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38205 La Laguna, Tenerife, Spain
3Dipartimento di Astronomia, Universit`a di Padova, vicolo Osservatorio, 3, 35122 Padova, Italy
4School of Physics and Astronomy, University of Nottingham, NG7 2RD, UK
5Herschel Science Centre, European Space Astronomy Centre, Villanueva de la Ca˜nada, 28691 Madrid, Spain
6Dept. of Physics & Astronomy, University of California, Irvine, CA 92697, USA
7Cardiff School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UK
8California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USA
9Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
10Space Science Building, Cornell University, Ithaca, NY, 14853-6801, USA
11Laboratoire d’Astrophysique de Marseille, OAMP, Universit´e Aix-marseille, CNRS, 13388 Marseille cedex 13, France
12Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK
13UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
14Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu - CNRS - Universit´e Paris Diderot, CE-Saclay, F-91191 Gif-sur-Yvette, France
15Dept. of Astrophysical and Planetary Sciences, CASA 389-UCB, University of Colorado, Boulder, CO 80309, USA
16Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
17Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
18Institute for Astronomy, University of Hawaii, Honolulu, HI 96822, USA
19Canada-France-Hawaii Telescope, Kamuela, HI, 96743, USA
20Astronomy Centre, Dept. of Physics & Astronomy, University of Sussex, Brighton BN1 9QH, UK
21Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK
22Space Science & Technology Department, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UK
23Institute for Space Imaging Science, University of Lethbridge, Lethbridge, Alberta, T1K 3M4, Canada
24Astrophysics, Oxford University, Keble Road, Oxford OX1 3RH, UK
25Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada
26Institut d’Astrophysique de Paris, UMR 7095, CNRS, UPMC Univ. Paris 06, 98bis boulevard Arago, F-75014 Paris, France
PP 010076
The chemical composition of the Orion star-forming region: II. Stars, gas, and dust: the abundance discrepancy conundrum
(1) Instituto de Astrofísica de Canarias
(2) Universidad de La Laguna
(3) Observatoire de Paris / Site du Meudon
PP 010075
On the Sensitivity of Partial Redistribution Scattering Polarization Profiles to Various Atmospheric Parameters
(1) IAC; (2) IAC, Univ. La Laguna and CSIC; (3) IAC and Univ. Firenze
PP 010074
High contrast optical imaging of companions: the case of the brown dwarf binary HD-130948BC
(1) Instituto de Astrofisica de Canarias, C/ Via Lactea s/n, La Laguna, Tenerife E-38200, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Islas Canarias, Spain
(3) Universidad Politecnica de Cartagena, Campus Muralla del Mar, Cartagena, Murcia E-30202, Spain
(4) Laboratoire de Physique Subatomique et de Cosmologie, 53 Avenue des Martyrs, 38026 Grenoble, France
(5) Max-Planck-Institut fr Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
(6) Consejo Superior de Investigaciones Cientificas, Spain.
PP 010072
Solid State radiolysis of amino acids in an astrochemical perspective
a Istituto Nazionale di Astrofisica—Osservatorio Astrofisica di Catania, Via S. Sofia 78, 95123 Catania, Italy
b Lupi Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy
c Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300, 00016 Monterotondo Stazione, Rome, Italy
d Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38200, La Laguna, Tenerife, Spain
e CSIC, Spain
PP 010071
Interpretation of HINODE SOT/SP asymmetric Stokes profiles observed in quiet Sun network and internetwork
(1) ESA/ESTEC, (2) Universita di Roma Tor Vergata, and (3) IAC
PP 010070
Magnetic fields and the outer rotation curve of M31
(1) IAC, (2) Departamento de Física Teórica y del Cosmos, Universidad de Granada, (3) Instituto de Física Teórica y Computacional Carlos I, Granada.
PP 010068
Interstellar C_2 in the Perseus molecular complex: excitation temperature and density of a molecular cloud with anomalous microwave emission.
Instituto de Astrofis\'{\i}ca de Canarias, 38200 La Laguna, Tenerife, Canary Islands, Spain
Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 010067
Aurorae Observed at the Canary Islands
(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, 06800, Mérida, Spain
(4) CGUL-IDL, Faculdade de Ciencias, Universidade de Lisboa, Ed. C-8, Campo Grande, 1749-016 Lisbon, Portugal
PP 010066
Formation of fullerenes in H-containing Planetary Nebulae
(1) IAC, (2) ULL, (3) CSIC, (4) ESAC-ESA, (5) NOAO, (6) UAM, (7) NCAC , (8) INSA-ESA
PP 010065
Characterization of Solar Telescope Polarization Properties Across the Visible and Near-Infrared Spectrum. Case Study: The Dunn Solar Telescope
(1) IAC, (2) National Solar Observatory/Sacramento Peak (USA)
PP 010064
The JCMT Nearby Galaxies Legacy Survey IV. Velocity Dispersions in the Molecular Interstellar Medium in Spiral Galaxies
McMaster Univ.; Univ. of Western Australia; Queen's University Kingston; IAC & ULL; etc.
PP 010063
The soft X-ray and narrow-line emission of Mrk573 on kiloparcec scales
(1) University of Crete, Department of Physics, Voutes, 71003 Heraklion, Crete, Greece
(2) Instituto de Astrofisica de Canarias, E-38200, La Laguna (SPAIN)
(3) Departamento de Astrofisica, Universidad de La Laguna, E-38205, La Laguna (SPAIN)
(4) Department of Physics & Astronomy, University of Sheffield, Sheffield, UK
PP 010062
AMINO ACIDS IN COMETS AND METEORITES: STABILITY UNDER GAMMA RADIATION AND PRESERVATION OF THE ENANTIOMERIC EXCESS
1Instituto de Astrofísica de Canarias (IAC), Via Lactea s/n, E-38200 La Laguna, Tenerife, Spain.
2Istituto Nazionale di Astrofisica. Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123
Catania, Italy.
3Actinium Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy.
4Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300, 00016 Monterotondo
Stazione, Rome, Italy.
5CSIC, Spain.
PP 010061
The Electrical Current Density Vector in the Inner Penumbra of a Sunspot
Instituto de Astrofísica de Canarias (IAC)
Departamento de Astrofísica, Universidad de La Laguna (ULL)
PP 010060
A geometrical height scale for sunspot penumbrae
Instituto de Astrofísica de Canarias
Departamento de Astrofísica, Universidad de La Laguna
PP 010059
CoRoT reveals a magnetic activity cycle in a Sun-like star
(1) CEA, (2) NCAR/HAO, (3) IAC, (4) ULL, (5) LATT Toulouse, (6) Obs. Paris
PP 010058
Mid-Infrared Galaxy Morphology from the Spitzer Survey of Stellar Structure in Galaxies (S^4G): The Imprint of the de Vaucouleurs Revised Hubble-Sandage Classification System at 3.6 microns
Alabama, IAC/ULL, etc.
PP 010057
The JCMT Nearby Galaxies Legacy Survey V: The CO(J=3-2) Distribution and Molecular Outflow in NGC~4631
Queens's University Kingston (Canada), IAC/ULL, etc
PP 010056
Decreased Frequency of Strong Bars in S0 Galaxies: Evidence for Secular Evolution?
Alabama, Oulu, IAC/ULL
PP 010055
Outburst activity in comets: II. A multi-band photometric monitoring of comet 29P/Schwassmann-Wachmann 1
(1) CSIC, (2) IEEC, (3) IAC, (4) ULL, (5) Gualba Astronomical Observatory, (6) La Cañada Observatory, (7) Uppsala University, (8) Guadarrama Observatory, (9) Observatorio Astronomico Municipal de Murcia
PP 010054
Observational evidence for a correlation between macroturbulent broadening and line-profile variations in OB Supergiants
(1) IAC, (2) ULL
PP 010053
Scattering Polarization of the Ca II IR Triplet for Probing the Quiet Solar Chromosphere
IAC
PP 010052
IPHAS extinction distances to Planetary Nebulae
(1) IAC, (2) Imperial College London, (3) University College London, (4) UNAM, (5) INT, (6) Macquarie University, (7) Karl-Franzens Universität, (8) Bristol University, (9) University of Manchester, (10) University of Hertfordshire, (11) Anglo-Australian Observatory, (12) ULL, (13) Centro Astronómico Hispano Alemán, (14) CEFCA.
PP 010051
Searching for the signatures of terrestial planets in solar analogs
Instituto de Astrofísica de Canarias
Centro de Astrofisica, Universidade do Porto
Observatoire Astronomique de l'Université de Genève
PP 010050
The complex structure of Abell 2345: a galaxy cluster with non–symmetric radio relics
(1) Fundacion Galileo Galilei, INAF, La Palma, Spain
(2) IAC
(3) DA, ULL
(4) Departamento de Astronomia, Univ. de Trieste (Italia)
(5) INAF, Osservatorio Astronomico di Trieste (Italia)
PP 010049
Low and High Temperature Infrared Spectroscopy of C60 and C70 Fullerenes
1IstitutoNazionale diAstrofisica – Osservatorio Astrofisico di Catania, Catania, Italy
2Actinium Chemical Research, Rome, Italy
3Instituto de Astrofisica de Canarias, Tenerife, Spain
PP 010048
Constraining the regular Galactic Magnetic Field with the 5-year WMAP polarization measurements at 22 GHz
(1) Universidad de Granada, (2) Instituto de Física Teórica y Computacional Carlos I (Granada), (3) IAC
PP 010047
Structural properties of disk galaxies. II. Intrinsic shape of bulges
((1) Instituto Astrofisico de Canarias,(2) Departamento de Astrofisica, Universidad de La Laguna, (3) Institut d'Astrophysique de Paris, C.N.R.S.-U.P.M.C., (4) Dipartimento di Astronomia, Universita di Padova)
PP 010046
Spectroscopy from Photometry Using Sparsity. The SDSS Case Study
Instituto de Astrofísica de Canarias
PP 010045
Thin discs, thick dwarfs and the effects of stellar feedback
(1) European Southern Observatory, (2) Instituto de Astrofısica de Canarias, (3) Departamento de Astrofısica, Universidad de La Laguna
PP 010044
A seismic signature of a second dynamo?
(1) Univ. Sheffield, (2) Univ. Birmingham, (3) IAC, (4) ULL, (5) Yale Univ., (6) CEA
PP 010043
Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry
KULeuven, LESIA-OPM, IAC, ULL
PP 010042
Exoplanet Status Report: Observation, Characterization and Evolution of Exoplanets and Their Host Stars
1 Space Research Institute (IWF), Austrian Academy of Sciences, Graz, Austria
2 Institute for Geophysics and Meteorology (IGAM), University of Graz, Austria
3 Observatoire ParisSite de Meudon LUTH, Paris, France
4 European Science Foundation, Standing Committee for Physical and Engineering Sciences, Strasbourg, France
5 Laboratoire de Planétologie de Grenoble CNRSUJF, Grenoble, France
6 Université de Bordeaux, France
7 Institut for Astronomy (INASAN), Russian Academy of Sciences, Moscow, Russia
8 Osservatorio Astronomico di Padova, INAF, Italy
9 Institute for Astronomy, University of Vienna, Vienna, Austria
10 Observatoiré de Paris—LESIA, Paris, France
12 ASTRON, Dwingeloo, The Netherlands
13 ETH Zürich Astrophysics Institute of Astronomy, Zürich, Switzerland
14 Instituto de Astrofisica de Canarias, Tenerife, Spain
15 The Swedish Institute of Space Physics, Kiruna, Sweden
16 Finish Meteorological Institute (FMI), Helsinki, Finland
17 Institute of Radio Astronomy in Kharkov of the Ukrainian Academy of Sciences, Ukraine
18 Space Research Institute (IKI), Russian Academy of Sciences, Moscow, Russia
19 Solar Geophysical Institute (PGI), Russian Academy of Sciences, Murmansk, Russia
20 Institute for Applied Physics (IAP), Russian Academy of Sciences, Nizhny Novgorod, Russia
21 Onsala Space Observatory Chalmers University of Technology, Onsala, Sweden
22 Universitát Göttingen, Institut für Astrophysik, Göttingen, Germany
23 Institut d’Estudis Espacials de Catalunya, Barcelona, Spain
24 Astrium Ltd, Stevenage, United Kingdom
25 The Hebrew University of Jerusalem, Jerusalem, Israel
26 INAF—Osservatorio Astronomico di Torino, Torino, Italy
27 Institut für Theoretische Physik und Astrophysik, Universitát zu Kiel, Kiel, Germany
PP 010041
The central region of M83: Massive star formation, kinematics, and the location and origin of the nucleus
(1) Instituto de Astrofisica de Canarias, E-38200 La Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, E-38205 La
Laguna, Tenerife, Spain
(3) Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia
(4) European Space Research & Technology Centre, Keplerlaan 1,
Postbus 299, 2200 AG Noordwijk, The Netherlands
(5) Stockholm Observatory, Department of Astronomy, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
(6) Oskar Klein Centre for Cosmoparticle Physics, Stockholm University,
SE-106 91 Stockholm, Sweden
(7)Universidad Nacional Autonoma de Mexico, Apartado
Postal 877, Ensenada, B.C. 22800, Mexico}
PP 010040
The kinematics of the quadrupolar nebula M 1–75 and the identification of its central star
1 Isaac Newton Group of Telescopes, Ap. de Correos 321, E-38700 Sta. Cruz de la Palma, Spaine-mail: msantander@ing.iac.es
2 Instituto de Astrof´ısica de Canarias, E-38200 La Laguna, Tenerife, Spain
3 Departamento de Astrof´ısica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
4 LAE, Universit´e de Montr´eal, C.P. 6128 Succ. Centre Ville, Montr´eal, QC H3C 3J7, Canada
5 Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester, M13 9PL, UK
6 Consejo Superior de Investigaciones Cient´ıficas, Madrid, Spain
7 Stockholm Observatory, Department of Astronomy, Stockholm University, AlbaNova, 106 91 Stockholm, Sweden
8 Centro de Astrobiolog´ıa, CSIC-INTA, Ctra de Torrej´on a Ajalvir km 4, E-28850 Torrej´on de Ardoz, Spain
9 Instituto de F´ısica de Cantabria (CSIC-Universidad de Cantabria), E-39005 Santander, Cantabria, Spain
10 Dpto. de F´ısica Moderna, Universidad de Cantabria, Avda de los Castros s/n, E-39005 Santander, Cantabria, Spain
PP 010039
A 33 GHz VSA survey of the Galactic plane from 27 to 46 degrees
Jodrell Bank Centre for Astrophysics, Univerity of Manchester
Instituto de Astrofísica de Canarias
Cavendish Laboratory, University of Cambridge
PP 010038
Multiple Major Outbursts from a Restless Luminous Blue Variable in NGC 3432
((1)Queen's University Belfast, (2) Max-Planck-Institut fuer Astrophysik, (3)
University of Turku, (4) Stockholm University, (5) Nordic Optical Telescope,
(6) Spitzer Science Center, (7) INAF Osservatorio Astronomico di Padova, (8)
Moonbase Observatory, (9) Sandvretens Observatory, (10) Instituto de
Astrofisica de Canarias, (11) Consejo Superior de Investigaciones Cienticas
of Spain, (12) Fundacion Galileo Galilei - INAF, (13) Armagh Observatory,
(14) Large Binocular Telescope Observatory)
PP 010037
A search for interstellar anthracene toward the Perseus anomalous microwave emission region
Instituto de Astrofisíca de Canarias, 38200 La Laguna, Tenerife, Canary Islands, Spain;
Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain;
Consejo Superior de Investigaciones Científicas, Spain;
Dpto. de Astrofísica y Ciencias de la Atmósfera, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040
Madrid, Spain;
The W.J. McDonald Observatory, University of Texas, Austin, TX 78712-1083, USA
PP 010036
Long-term changes in insolation and temperatures at different altitudes
Instituto de Astrofisica de Canarias, Via Lactea s/n, E38200, La Laguna, Spain
Climate Research Laboratory, Barcelona Science Park, Barcelona, Spain
PP 010035
An improved method for statistical studies of the internal kinematics of HII regions: the case of M83
1. Observatorio de Estocolmo, Suecia. 2. IAC, 3. CSIC. 4. ULL, 5. UNAM, Ensenada, México, 6. Observatorio de Marsella, Francia. 7. Dept. Astronomía, U. Montreal,
Canada
PP 010033
Image Reconstruction with Analytical Point Spread Functions
(1) Instituto de Astrofisica de Canarias, (2) THEMIS, CNRS UPS 853
PP 010032
A Detailed Look at Chemical Abundances in Magellanic Cloud Planetary Nebulae. I. The Small Magellanic Cloud
(1) NOAO; (2) Western Kentucky University; (3) IAC; (4) Univ. La Laguna; (5) Herschel Science Centre-ESAC; (6) ESAC-INSA; (7) Univ. Auton. Madrid; (8) CSIC; (9) Weber State University; (10) Univ. of Washington
PP 010031
The solar-like CoRoT target HD 170987: spectroscopic and seismic observations
(1) CEA, France, (2) HAO/NCAR, USA, (3) IAC
PP 010030
Bars do drive spiral density waves
(1) Univ. of Oulu, (2) Univ. of Alabama, (3) IAC, (4) Univ. de La Laguna
PP 010029
Internal dynamics of Abell 2294: a massive, likely merging cluster
(1) Univ. di Trieste, Trieste, Italia
(2) Osservatorio Astronomico di Trieste, Trieste, Italia
(3) Fundacion Galileo- Galilei, INAF, España
(4) IAC, España
(5) Dep. de Astrofosica, ULL, España
PP 010028
Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System
(1) IAC, (2) Departamento de Astrofísica, ULL, (3) CEFCA, (4) UCM, (5) Kapteyn Astronomical Institute
PP 010027
GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
(1) IAC
(2) Departamento de Astrofisica, Universidad de La Laguna
(3) Dipartimento di Astronomia, Universita' di Padova
PP 010026
Acoustic power absorption and enhancement generated by slow and fast MHD waves
(1) PMOD/WRC Davos, (2) CEA Paris, (3) IAC, (4) University of Birmingham, UK, (5) Max-Planck Institute, Germany
PP 010025
Study of star-forming galaxies in SDSS up to redshift 0.4 II. Evolution from the fundamental parameters: mass, metallicity & SFR
Instituto de Astrofisica de Canarias, 38200 La Laguna, Spain
Departamento de Astrofisica, Universidad de la Laguna, Spain
Departamento de Fisica, Escuela Superior de Fisica y Matematica, IPN, Mexico D.F., Mexico
Herschel Science Center, INSA/ESAC, Madrid, Spain
PP 010024
A New Gas Cell for High-Precision Doppler Measurements in the Near-Infrared
(1)IAC,(2)ULL,(3)CAB,(4)UCF
PP 010023
Magnetic bright points in the quiet Sun
(1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain
(3) ESA/ESTEC RSSD, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
(4) Dipartimento di Fisica, Universita degli Studi di Roma Tor Vergata, Rome, Italy
PP 010022
Small-spatial scale variations of nebular properties and the abundance discrepancy in three Galactic HII regions
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Spain
PP 010021
The impact of enhanced He and CNONa abundances on globular cluster relative age-dating methods.
(1) IAC, (2) Osservatorio Astronomico di Teramo.
PP 010019
The evolutionary sequence of sub-mm galaxies: from diffuse discs to massive compact ellipticals?
(1) IAC, (2) Departamento de Astrofisica, Universidad de La Laguna
(3) School of Physics and Astronomy, University of Nottingham
PP 010018
The redshift and broad band spectral energy distribution of NRAO 150
1-Instituto de Astrofisica de Canarias, E-38200 La Laguna
2-Departamento de Astrofisica Universidad de La Laguna, E-38205 La Laguna
3-Instituto de Astrofisica de Andalucia, E-18080 Granada
4-Institute for Astrophyisical Research, Boston University, Boston MA02215 - USA
5-Department of Physics & Astronomy, University of Shefield, UK
6-Isaac Newton Group of Telescopes, La Palma
PP 010017
Automatic unsupervised classification of all SDSS/DR7 galaxy spectra
(1) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, E-38071 La Laguna,
Tenerife, Spain
PP 010016
Small magnetic loops connecting the quiet surface and the hot outer atmosphere of the Sun
IAC, IAC, IAC, IAA
PP 010015
Oxygen isotopic ratios in cool R Coronae Borealis stars
(1) Instituto de Astrofisica de Canarias, (2) W. J. McDonald Observatory, (3) Indian Institute of Astrophysics, (4) National Optical Astronomy Observatory, (5) Department of Physics and Astronomy, Uppsala University
PP 010014
New groups of planetary nebulae with peculiar dust chemistry towards the Galactic bulge
(1) N. Copernicus Astronomical Center, (2) ESAC-ESA, (3) Instituto de Astrofisica de Canarias
PP 010013
Gemini K-band NIRI Adaptive Optics Observations of Massive Galaxies at 1 < z < 2
(1) Gemini Observatory/AURA, (2) U. of Nottingham, (3) Instituto de Astrofisica de Canarias
PP 010012
Which Galaxies Host Bars and Disks? A Study of the Coma Cluster
(1)Instituto de Astrofísica de Canarias
(2)Departamento de Astrofísica, Universidad de La Laguna
(3)European Southern Observatory
PP 010011
Photometric scaling relations of lenticular and spiral galaxies
Univ. of Oulu, univ. of Oulu, Univ. of Alabama, IAC, IAC
PP 010010
Statistical analysis of the very quier Sun magnetism
Instituto de Astrofísica de Canarias
THEMIS
Istituto Richerche Solari Locarno
Institute of Academy, ETH Zurich
PP 010009
Gauss-Seidel and Successive Overrelaxation Methods for Radiative Transfer with Partial Frequency Redistribution
IAC
PP 010008
Absence of significant cross-correlation between WMAP and SDSS
1. IAC; 2 ULL; 3 Centro Studi e Ricerche Enrico Fermi, Via Panisperna 89 A, Compendio del Viminale, 00184 Rome, Italy; 4 Istituto dei Sistemi Complessi CNR, Via dei Taurini 19, 00185 Rome, Italy
PP 010007
On the Probable Existence of an Abrupt Magnetization in the Upper Chromosphere of the Quiet Sun
IAC
PP 010005
Explaining the Galactic Interstellar Dust Grain Size Distribution Function
Instituto de Astrofisica de Canarias
Department of Astrophysics University of La Laguna
PP 010004
The asteroseismic potential of Kepler: first results for solar-type stars
(1) University of Birmingham, (2) IAC, (3) ULL, (4) CEA-Paris
PP 010003
Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
(1) IAC, (2) CITA, (3) MPA, (4) Department of Physics, UIUC, (5) Center for Advanced Studies, UIUC
PP 010002
The Galaxy-wide distributions of mean electron density in the HII regions of M51 and NGC4449
(1) UNAM, Ensenada, Mexico. (2) IAC (3) CSIC (4) ULL
PP 010001
A study of the galaxy redshift distribution toward the cosmic microwave background cold spot in the Corona Borealis supercluster
(1) Instituto de Astrofísica de Canarias
(2) Universidad de La Laguna
(3) Consejo Superior de Investigaciones Científicas