Preprints in 2011
PP 011081
Analysis of chemical abundances in planetary nebulae with [WC] central stars. I. Line intensities and physical conditions
(1) IAC, (2) Dep. Astrofísica. U. La Laguna, (3) IA-UNAM, Mexico, (4) Dep. Astronomía, U. Chile
PP 011080
The Ly-alpha Lines of H I and He II: A Differential Hanle Effect for Exploring the Magnetism of the Solar Transition Region
IAC
PP 011079
Scattering Polarization and Hanle Effect in Stellar Atmospheres with Horizontal Inhomogeneities
IAC
PP 011078
The Impact of Quantum Interference between Different J-levels on Scattering Polarization in Spectral Lines
IAC
PP 011077
Center-to-limb variation of the area covered by magnetic bright points in the quiet Sun
((1) Instituto de Astrofisica de Canarias, Tenerife,Spain,
(2) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain
(3) Image Processing Laboratory, Universidad de Valencia, Spain)
PP 011076
VVV DR1: The First Data Release of the Milky Way Bulge and Southern Plane from the Near-Infrared ESO Public Survey VISTA Variables in the Via Lactea
(1) Departamento Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Santiago, Chile
(2) IAC
PP 011075
Overview of the Near-IR S0 galaxy Survey (NIRS0S)
U. Oulu & FINCA, U. Oulu, U. Alabama, IAC & ULL
PP 011074
Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: I. Correcting for contamination by PAH, hot dust, and intermediate age stars
MPIA, IAC, ULL, etc.
PP 011073
A Strong Dichotomy in S0 Disk Profiles Between the Virgo Cluster and the Field
((1)Max-Planck-Institut fuer extraterrestrische Physik, Garching, Germany,
(2) UNAM, Instituto de Astronomia, Ensenada, Mexico,
(3) Instituto de Astrofisica de Canarias, La Laguna, Spain)
(4) CSIC
(5) Dept. Astrofísica Ull.
PP 011072
The age of extremely red and massive galaxies at very high redshift
Instituto de Astrofísica de Canarias (IAC); Departamento de Astrofísica, Universidad de La Laguna.
PP 011071
Constraining the formation of inner bars. Photometry, kinematics and stellar populations in NGC 357
(1) IAC, (2) Depto. Astrofísica, ULL, (3) Dipartimento Astronomia, Universita di Padova, (4) Jeremiah Horrocks Institute, University of Central Lancashire
PP 011070
Near-IR Atlas of S0-Sa galaxies (NIRS0S)
1 Dept. of Physics/Astronomy Division, University of Oulu, FI-90014 Finland
2 Finnish Centre of Astronomy with ESO (FINCA), University of Turku, V ̈aisa ̈l ̈antie 20, FI-21500, Piikki ̈o, Finland
3 Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487
4 Instituto de Astrof ́ısica de Canarias, E-38200 La Laguna, Tenerife, Spain
5 Departamento de Astrof ́ısica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 011069
Reconstructing the photometric light curves of Earth as a planet along its history
(1) IAC, (2) ULL
PP 011068
The ACS LCID project VII: the blue stragglers population in the isolated dSph galaxies Cetus and Tucana
(1)IAC, (2)ULL (3)INAF-Teramo Obs. (4)INAF-Padova Obs (5)Royal Obs. of Edinburgh (6)Univ of Minnesota (7)DAO-HIA (8)Univ. of Zurich (9)Kapteyn Astron. Inst.
PP 011067
Internal dynamics of Abell 2254: a merging galaxy cluster with a clumpy, diffuse radio emission
(1) Univ. di Trieste (Italia)
(2) INAF. Osservatorio Astronomico di Trieste (Italia)
(3) INAF. Osservatorio Astronomico di Bologna (Italia)
(4) IAC, ULL
(5) INAF, TNG, Fundacion Galileo Galilei
(6) INAF-IASF, Milano (Italia)
PP 011066
Fossil groups origins II. Unveiling the formation of the brightest group galaxies through their scaling relations
(1) Instituto Astrofisico de Canarias, (2) Departamento de Astrofisica, (3) European Southern Observatory, (4) Fundacion Galileo Galilei-INAF, (5) Dipartimento di Astronomia, Universita di Padova, (6) UNINOVA/CA3, (7) Harvard-Smithsonian Center for Astrophysics, (8) Dipartimento di Fisica-Sezione Astronomia, Universita degli Studi di Trieste, (9) INAF-Osservatorio Astronomico di Trieste, (10) Instituto de Astrofisica de Andalucia-C.S.I.C., (11) Centro Astronomico Hispano Aleman, (12) INAF-Osservatorio Astronomico di Capodimonte
PP 011065
Looking for a connection between the Am phenomenon and hybrid delta Sct/gamma Dor pulsation: a determination of the fundamental parameters and abundances of HD 114839 and BD +18 4914
(1) Uni. Vienna, (2) Open University Milton Keynes, (3) IAA-CSIC, (4) Kiepenheuer Institut fuer Sonnenphysik, (5) IAC, (6) ULL, (7) INAF-OAB Merate
PP 011064
The excitation of solar-like oscillations in a delta Sct star by efficient envelope convection
(1) Uni. Vienna, (2) Copernicus Astronomical Center, (3) Uni. Porto, (4) Uni. Aarhus, (5) NOT, (6) CAB INTA-CSI, (7) Uni. British Columbia, (8) KULeuven, (9) Uni. Sydney, (10) INAF-Catania, (11) ROB, (12) CEA Saclay, (13) KIS, (14) IAC, ULL, (15) UCLAN, (16) SETI institute, NASA Ames, (17) Orbital Sciences Corporation, NASA Ames
PP 011063
Resonant structure in the disks of spiral galaxies, using phase-reversals in streaming motions from 2D Hα Fabry-Perot spectroscopy
1. Instituto de Astrofísica de Canarias 2. Departamento de Astrofísica, ULL.
3. CSIC 4. Laboratoire d’Astrophysique de Toulouse-Tarbes. Université de Toulouse, CNRS 5. CNRS, IRAP 7. Oscar Klein Centre for Cosmoparticle Physics, Stockholm University 8. Instituto de Astronomía, UNAM, Ensenda. 9. Département de Physique et Astronomie, Université de Montreal,
PP 011061
Angular momentum transfer between oscillations and rotation in subdwarf B hybrid pulsators
(1) IAC (2) IAA (3) Institute of Astronomy, Cambridge
PP 011060
Detection of anomalous microwave emission in the Pleiades reflection nebula with WMAP and the COSMOSOMAS experiment
(1) Instituto de Astrofísica de Canarias
(2) Departamento de Astrofísica, Universidad de La Laguna
(3) Consejo Superior de Investigaciones Científicas
(4) California Institute of Technology
PP 011059
The Galactic IMF: origin in the combined mass distribution functions of dust grains and gas clouds
(1) IAC (2) Dept. Astrofísica ULL. (3) CSIC)
PP 011058
The orbital phases and secondary transit of Kepler-10b - A physical interpretation based on the Lava-ocean planet model
(1) LESIA, (2) IAC, (3) ULL, (4) IAP, (5) I. Astr. Spatiale Paris, (6) Washington U.
PP 011057
The HARPS search for southern extra-solar planets XXXII. Only 4 planets in the Gl 581 system
(1) U. Grenoble, (2)U Hawaii, (3) Obs. Geneva, (4) IAP, (5) OHP, (6) U. Liege, (7) U. Porto, (8) U. Porto, (9) LAM, (10) IAC, (11) ULL, (12) U. Catol. Chile
PP 011055
Using Stellar Densities to Evaluate Transiting Exoplanetary Candidates
(1) IAC, (2)Obs. Marseille, (3) IAC
PP 011054
Systematic search for extremely metal poor galaxies in the Sloan Digital Sky Survey
IAC, Departamento Astro. ULL
PP 011052
A Petal of the Sunflower: Photometry of the Stellar Tidal Stream in the Halo of Messier 63 (NGC 5055)
University of Texas, University of Virgina, MPIA, IAC, Blackbird Observatory, Sirius Imaging Observatory
PP 011051
Chemical abundance analysis of the open clusters Berkeley 32, NGC 752, Hyades, and Praesepe
(1) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain
(3) INAF-Osservatorio Astronomico di Bologna, Bologna, Italy
(4) Centro de Investigaciones de Astronomía, Mérida, Venezuela
PP 011050
Orbit Determination of Close Binary Systems using Lucky Imaging
(1) Astronomical Society of Mérida, C/Toledo, no 1 Bajo, Mérida, E-06800, Spain
(2) Double Star Section of LIADA, S3000ZAA Santa Fe, Argentina
(3) IAC, ULL-DA
(4) Astronomical Observatory MPC J-48, E-38205, Spain
(5) Grupo de Observadores Astronómicos de Tenerife (GOAT), Spain
(6) Astronomical Society of Isla de la Palma, E-38712, Spain
PP 011049
Detection of Infalling Hydrogen in transfer between between the interacting galaxies NGC 5426 and NGC5427
1. IAC, (2) Dept. Astrofísica ULL (3) CSIC, (4) UNAM, México DF. (5) Lab. d'Astrophysique Toulouse-Tarbes. (6) CNRS, IRAP, Toulouse. (7) Dept. Astronomy. U.Stockholm, (8) Oscar Klein Centre, Stockholm., (9) Dept. Physique et Astronomie,U. Montreal. (10). Dept. Astronomy, U. Cape Town (11) UNAM, Ensenada,
(12).Dept. Fis. Teorica y del Cosmos, U. Granada., (13). Dept Física, Escuela Sup. Fis. Mat. IPN, UP Adolfo Lopez Mateos. México.
PP 011048
The Outer Disks of Early-type Galaxies, II. surface Brightness Profiles of Unbarred Galaxies, and Trends with Hubble Type
1. UNAM, Ensenada Mexico, 2. IAC, 3. Max Planck Institut fúr Extraterrestresche Physic, Garching. (4) Universität-Sternwarte, München. 5. Guest Investigator of the UK Astronomy Data Centre. 6. Present Address, Dept. Phys. Astronomy, UCL (London), 7. Facultad de Física, ULL. 8. CSIC.
PP 011047
The Hanle Effect of the Hydrogen Ly-alpha Line for Probing the Magnetism of the Solar Transition Region
(1) IAC, (2) High Altitude Observatory, NCAR-Boulder
PP 011045
Nuclear Rings in Galaxies---A Kinematic Perspective
NASA-GSFC; Maryland; IAC & ULL; Maryland
PP 011044
Grand Design and Flocculent Spirals in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
Vassar College, IAC, ULL, others
PP 011043
The SAURON Project - XIX. Optical and near-infrared scaling relations of nearby elliptical, lenticular and Sa galaxies
(1) IAC, (2) ULL, (3) ESA/ESTEC, (4) MPIA, (5) IAS, (6) RUG, (7) Oxford University, (8) Korea Astronomy and Space Science Institute, (9) Yonsei University Observatory, (10) CRAL, (11) ESO, (12) STRW, (13) STECF/ESO, (14) Gemini Observatory, (15) University of Hertfordshire, (16) University of California-Berkeley, (17) Northrop Grumman Aerospace Systems, (18) University of Toronto, (19) Yonsei University
PP 011042
An updated MILES stellar library and stellar population models
(1) IAC, (2) ULL, (3) UAM, (4) UCM, (5) CEFCA, (6) RUG
PP 011041
Bayesian Magnetohydrodynamic Seismology of Coronal Loops
(1) Departament de Física, Universitat de les Illes Balears
(2) Instituto de Astrofísica de Canarias
(3) Departamento de Astrofísica, Universidad de La Laguna
PP 011040
Resolving the nuclear dust distribution of the Seyfert 2 galaxy NGC 3081
(1) Univ. Sheffield, (2) Herschel Science Centre, (3) IAC, (4) ULL, (5) IFC, (6) CAB, (7) ESO, (8) IAA, (9) Univ. Florida
PP 011039
The formation of fullerenes: clues from new C60, C70, and (possible) planar C24 detections in Magellanic Cloud Planetary Nebulae
(1) IAC; (2) ULL; (3) CSIC; (4) ESAC-ESA; (5) NOAO; (6) UAM; (7) INA; (8) ACR
PP 011038
The Kepler characterization of the variability among A- and F-type stars I. general overview
(1) Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot; CEA, IRFU, SAp, Centre de Saclay, 91191, Gif-sur-Yvette, France , (2) Kiepenheuer-Institut fur Sonnenphysik, Schoneckstrasse 6, 79104 Freiburg im Breisgau, Germany, (3) Instituto de Astrofisica de Canarias, 38200 La Laguna, Tenerife, Spain; Departamento de Astrofisica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain, (4) Laboratorio de Astrofisica Estelar y Exoplanetas, LAEX-CAB , (INTA-CSIC), PO BOX 78, 28691 Villanueva de la Canada, Madrid, Spain, (5) Centro de Astrofisica, Faculdade de Ciencias, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal, (6) Los Alamos National Laboratory, XTD-2, Los Alamos, NM 87545-2345, USA, (7) Instituto de Astrofisica de Andalucia , (CSIC), Apartado 3004, 18080 Granada, Spain, (8) LESIA, Observatoire de Paris, CNRS, UPMC, Universite Paris-Diderot, 92195 Meudon, France, (9) Valentian International University, Prolongacion C/ Jose Pradas Gallen, s/n 12006 Castellon de la Plana - Spain, (10) Astrophysics Group, Keele University, Staffordshire, ST5 5BG, United Kingdom, (11) Institut fur Astronomie, Turkenschanzstrasse 17, 1180 Wien, Austria, (12) Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland, (13) South African Astronomical Observatory, P.O. Box 9, Observatory 7935, South Africa, (14) Instytut Astronomiczny, Uniwersytet Wroclawski, Kopernika 11, 51-622 Wroclaw, Poland, (15) Observatorio Astronomico Nacional, Instituto de Astronomia, UNAM, Ensenada B.C., Apdo. Postal 877, Mexico , (16) CISAS, Padova University, Via Venezia 15, 35131 Padova, Italy, (17) INAF - Astronomical Observatory of Padova, Vicolo Osservatorio 5, 35122 Padova, Italy, (18) UMR 6525 H. Fizeau, UNS, CNRS, OCA, Campus Valrose, 06108 Nice Cedex 2, France, (19) Instituut voor Sterrenkunde, K.U.Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium, (20) Konkoly Observatory of the Hungarian Academy of Sciences, 1525 Budapest PO Box 67, Hungary, (201) INAF - Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, (22) Lab. d'Astrophysique de Toulouse-Tarbes, Universite de Toulouse, CNRS, 57 avenue d'Azereix, 65000 Tarbes, France , (23) Thuringer Landessternwarte Tautenburg, 07778 Tautenburg, Germany , (24) Department of Astronomy, New Mexico State University, Las Cruces, NM 88001, USA , (25) Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands, (26) University of Birmingham, School of Physics and Astronomy, Edgbaston, Birmingham B15 2TT, UK , (27) Department of Astronomy and Physics, Saint Marys University, Halifax, NS B3H 3C3, Canada , (28) Observatoire de Geneve, Universite de Geneve, 51 ch. des Maillettes, 1290 Sauverny, Switzerland , (29) Los Alamos National Laboratory, XCP-6, MS T-087, Los Alamos, NM 87545-2345, USA , (30) Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire, Preston PR12HE, UK , (31) Royal Observatory of Belgium, Ringlaan 3, 1180 Brussel, Belgium , (32) Department of Physics and Astronomy, University of Aarhus, bygn. 1520, Ny Munkegade, 8000 Aarhus C., Denmark , (33) Department of Astronomy, University of Texas, Austin, TX78712, USA , (34) Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW, 2006, Australia , (35) Bay Area Environmental Research Inst./NASA Ames Research Center, Moffett Field, CA 94035, USA , (36) SETI Institute/NASA Ames Research Center, Moffett Field, CA 94035, USA
PP 011037
Dust around R Coronae Borealis stars: I. Spitzer/IRS observations
(1) IAC; (2) ULL; (3) Indian Institute of Astrophysics; (4) W. J. McDonald
Observatory, UT
PP 011036
Chemical Abundances of the Secondary Star in the Black Hole X-Ray Binary V404 Cygni
(1)Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain
(2)Depto. AstrofÃísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
(3)Consejo Superior de Investigaciones Científicas, Spain
(4)Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA
(5)Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
PP 011035
Long-term evolution of the aerosol debris cloud produced by the 2009 8impact on Jupiter
(1) Departamento de fisica Aplicada I, Escuela Tecnica Superior de Ingenieria, Universidad del Pais Vasco, Bilbao, Spain
(2) Instituto de Astrofisica de Canarias, E-38200, La Laguna, Tenerife, Spain
(3) Departamento de Astrofisica, Universidad de La Laguna, E-38205, La Laguna, Tenerife, Spain
PP 011034
Integral field spectroscopy of selected areas of the Bright Bar and Orion-S cloud in the Orion Nebula
Instiruro de Astrof'isica de Canarias, E-38200, La Laguna, Tenerife, Spain
Departamento de Astrof'isica. Universidad de La Laguna, E-38205, La Laguna, Tenerife, Spain
PP 011033
Metallicities, Age--Metallicity relationships, and Kinematics of Red Giant Branch Stars in the Outer Disk of the Large Magellanic Cloud
(1) Instituto de Astrofisica de Canarias, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, Spain, (3) National Radio Astronomy Observatory, Chile, (4) Departamento de Astronomia, Universidad de Chile, Chile
PP 011032
Evidence of a Distinct Stellar Population in the Counterrotating Core of NGC 1700
Instituto de Astrofísica de Canarias, E38200 La Laguna, Tenerife, Spain
Departamento de Astrofísica, Universidad de La Laguna, E38205 La Laguna, Tenerife, Spain
Departamento de Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, E28049 Madrid, Spain
PP 011031
The impact of the Kasatochi eruption on the Moons illumination during the August 2008 lunar eclipse
(1) Instituto de Astrofisica de Canarias (IAC), C/ Via Lactea s/n, E-38200 La
Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
(3) Centro de Astrobiologia, CSIC-INTA,
PP 011030
Constraints on the Polarization of the Anomalous Microwave Emission in the Perseus Molecular Complex from 7-year WMAP data.
Instituto de Astrofísica de Canarias (IAC)
Dpto. Astrof'isica, Universidad de La Laguna (ULL)
PP 011029
Atmospheric optical-turbulence at Roque de los Muchachos Observatory: database and recalibration of the generalized-SCIDAR data
1 Instituto de Astrofisica de Canarias
2 Dept. Astrofisica, Universidad de La Laguna
PP 011028
Search and characterization of T-type planetary mass candidates in the Sigma Orionis cluster
(1)Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain. e-mail:karla@iac.es
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain.
(3) Centro de Astrobiología (CSIC-INTA), E-28850 Torrejón de Ardoz, Madrid, Spain.
(4) Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain.
(5) Leibniz Institute for Astrophysics Potsdam, An der Sternwarte 16, D-14482 Potsdam,
Germany.
PP 011027
Radiolysis and radioracemization of 20 amino acids from the beginning of the Solar System
F. Cataldo (&)
Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Catania, Via S. Sofia 78,95123 Catania, Italy
F. Cataldo
Lupi Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy
O. Ursini G. Angelini
Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300,
Monterotondo Stazione, 00016 Rome, Italy
S. Iglesias-Groth , A. Manchado
Instituto de Astrofísica de Canarias (IAC), Via Lactea s/n,
38200 La Laguna, Tenerife, Spain
A. Manchado CSIC, Madrid, Spain
PP 011026
A global study of the HII region M43 and its ionizing star (I. Stellar parameters and nebular empirical analysis)
(1) IAC, (2) ULL, (3) OPM, (4) AAO , (5) UNAM,
PP 011025
The chemical composition of the Orion star-forming region. III. C, N, Ne, Mg and Fe abundances in B-type stars revisited
(1) MPI, (2) IAC, (3) ULL
PP 011024
Determining the Magnetization of the Quiet Sun Photosphere from the Hanle Effect and Surface Dynamo Simulations
Main Astronomical Observatory;
Instituto de Astrofisica de Canarias
PP 011023
Infrared and optical polarimetry around the low-mass star-forming region NGC1333 IRAS 4A
(1)Institut de Ci`encies de l'Espai (IEEC-CSIC), Facultat de Ciéncies, 08193 Bellaterra, Catalunya, Spain
(2) Instituto de AstrofÃsica de Canarias, Vía Láctea s/n, E-38200 La Laguna, Tenerife, Spain
(3) Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
(4) Departamento de Física - ICEx - UFMG, Caixa Postal 702, 30.123-970 Belo Horizonte, Brazil
(5) Departament d'Astronomia i Meteorologia (IEEC-UB), Institut de Ciencies del Cosmos,
Universitat de Barcelona, Martí i Franquès 1, E-08028 Barcelona, Spain
PP 011022
Are Solar Chromospheric Fibrils Tracing the Magnetic Field?
Department of Astronomy, Stockholm University
IAC
PP 011021
Dissecting the size evolution of elliptical galaxies since z~1: Puffing up vs minor merging scenarios
(1) IAC, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) Mullard Space Science Laboratory, (4) Department of Physics and Astronomy, University College London
PP 011020
Relationship between Hubble type and spectroscopic class in local galaxies
Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain (1),
Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain (2),
GEPI, Paris-Meudon Observatory 5, Place Jules Janssen, Meudon, Paris,
France (3), Universite Paris Diderot, Paris Cedex 13, France (4)
PP 011019
Blue luminous stars in nearby galaxies - UIT005: a possible link to the Luminous Blue Variable stage
(1) UH Institute for Astronomy (2) IAC & Universidad de La Laguna (3) ESA, Space Telescope Science Institute, (4) Universidad de Guadalajara, (5) Geneva Observatory
PP 011018
Lunar eclipse theory revisited: Scattered sunlight in both the quiescent and the volcanically perturbed atmosphere
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain
Department of Astrophysics, Faculty of Physics, Universidad de La Laguna, Tenerife, Spain
PP 011017
Do galaxies form a spectroscopic sequence?
(1) Universidad Autonoma de Madrid, Spain, (2) IAC
PP 011016
A detailed analysis of the properties of radiolyzed proteinaceous amino acids
The top down approach in the search of the origins of life
F. Cataldo (&)
has involved the analysis of meteorites and in particular of
Istituto Nazionale di Astrofisica. Osservatorio Astrofisico di
the carbonaceous chondrites (CC). Indeed a plethora of
Catania, Via S. Sofia 78, 95123 Catania, Italy
different classes of molecules have been identified in
e-mail: franco.cataldo@fastwebnet.it
meteorites since long time [1]. The most impressive class
F. Cataldo
of molecules identified yet regards the amino acids which
Lupi Chemical Research, Via Casilina 1626/A,
are the basic molecules used in the current terrestrial bio-
00133 Rome, Italy
chemistry. Not only a considerable number of different
P. Ragni amino acids have been identified in CC [2], but part of
Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300,
them were also detected in enantiomeric excess [3–6]. This
00016 Monterotondo Stazione, Rome, Italy
S. Iglesias-Groth à A. Manchado
Ì
Instituto de Astrofısica de Canarias (IAC), Via Lactea s/n, before the formation of the Solar System [7] but also
38200 La Laguna, Tenerife, Spain
F. Cataldo.
Istituto Nazionale di Astrofisica. Osservatorio Astrofisico diCatania, Via S. Sofia 78, 95123 Catania, Italy
e-mail: franco.cataldo@fastwebnet.it
F. Cataldo
Lupi Chemical Research, Via Casilina 1626/A,
P. Ragni Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300,00016 Monterotondo Stazione, Rome, Italy
S. Iglesias-Groth à A. Manchado
Instituto de Astrofısica de Canarias (IAC), Via Lactea s/n, before the formation of the Solar System [7] but also
38200 La Laguna, Tenerife, Spain
A. Manchado
CSIC, Madrid, Spain
A. Manchado
light on racemic mixtures [8].
CSIC, Madrid, Spain
PP 011015
Solid state radiolysis of sulphur-containing amino acids: cysteine, cystine and methionine
F. Cataldo (&)
Istituto Nazionale di Astrofisica, Osservatorio Astrofisico meteorite [1, 2].
di Catania, Via S. Sofia 78, 95123 Catania, Italy
e-mail: franco.cataldo@fastwebnet.it
Lupi Chemical Research, Via Casilina 1626/A, 00133 Rome,
Italy
P. Ragni
Istituto di Metodologie Chimiche, CNR, Via Salaria
Km 29,300, 00016 Monterotondo Stazione, Rome, Italy
S. Iglesias-Groth, A. Manchado
Instituto de Astrofu0131sica de Canarias (IAC), Via Lactea s/n, 38200 La Laguna, Tenerife, Spain
PP 011014
Asymmetries of the Stokes V profiles observed by HINODE SOT/SP in the quiet Sun
(1) ESA/ESTEC RSSD, Noordwijk, The Netherlands, (2) IAC
PP 011012
Unnoticed magnetic field oscillations in the very quiet Sun revealed by Sunrise/IMaX
(1) IAC
(2) Depto. Astrofisica ULL
(3) MPS
(4) THEMIS
(5) KIS
PP 011011
Scattering Polarization of Hydrogen Lines in Weakly Magnetized Stellar Atmospheres I. Formulation and Application to Isothermal Models
IAC
PP 011010
Infrared spectroscopy and integrated molar absorptivity of C60 and C70 fullerenes at extreme temperatures
Instituto 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
4Consejo Superior de Investigaciones Científicas, Spain
5Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 011009
On the inversion of Stokes profiles with local stray-light contamination
IAC
Departamento de Astrofisica, ULL
PP 011008
Bayesian inference of solar and stellar magnetic fields in the weak-field approximation
Instituto de Astrofisica de Canarias
PP 011007
CHARACTERIZING THE ATMOSPHERES OF TRANSITING ROCKY PLANETS AROUND LATE-TYPE DWARFS
1. IAC
2. ULL
3. CAB
PP 011006
Testing the Unification Model for AGN in the Infrared: are the obscuring tori of Type 1 and 2 Seyferts different?
(1) Univ. Sheffield, (2) Gemini Observatory (La Serena), (3) CAB, (4) IAC, (5) ULL, (6) Univ. Florida, (7) Gemini Observatory (Hilo), (8) Univ. Crete
PP 011005
Far-infrared imaging of post-AGB stars and (proto)-planetary nebulae with the AKARI Far-Infrared Surveyor
(1) Institute of Astronomy, K.U.Leuven (2) IAC; (3) ULL; (4) ESAC-ESA; (5) CSIC
PP 011004
Are C60 molecules detectable in circumstellar shells of R Coronae Borealis stars?
(1) IAC; (2) ULL; (3) Indian Institute of Astrophysics; (4) W. J. McDonald Observatory, UT
PP 011003
Clear detection of dusty torus signatures in a Weak-Line Radio Galaxy: the case of PKS 0043-42
(1) Department of Physics and Astronomy, Univ. Sheffield
(2) Department of Physics and Astronomy, Rochester Institute of Technology
(3) Instituto de Astrofisica de Canarias
(4) Departamento de Astrofisica, Univ. La Laguna
(5) Max-Planck Institute für Astronomie
(6) School of Physics, Astronomy and Mathematics, Univ. Hertfordshire
PP 011002
A High-Resolution Three-Dimensional Model of the Solar photosphere Derived from Hinode Observations
IAC
PP 011001
IRAS 17423-1755 (Hen 3-1475) revisited: an O-rich high-mass post-Asymptotic Giant Branch Star
(1) Universidade da Coruña; (2) IAC; (3) ULL; (4) Universidade de Vigo; (5) CSIC; (6) ESAC-ESA