SN 2005cs in M51 -II. Complete evolution in the optical and the near-infrared
- Author
- PASTORELLO, A1 ; VALENTI, S1 ; BIRTWHISTLE, P6 ; BOTTICELLA, M. T1 ; CAPPELLARO, E2 ; DEL PRINCIPE, M7 ; DI MILLE, F8 ; DI RICO, G7 ; DOLCI, M7 ; ELIAS-ROSA, N9 ; EFIMOVA, N. V10 4 ; FIEDLER, M11 ; ZAMPIERI, L2 ; HARUTYUNYAN, A12 2 ; HÖFLICH, P. A13 ; KLOEHR, W14 ; LARIONOV, V. M10 15 4 ; LORENZI, V12 ; MAUND, J. R16 17 ; NAPOLEONE, N18 ; RAGNI, M7 ; RICHMOND, M19 ; RIES, C5 ; NAVASARDYAN, H2 ; SPIRO, S1 18 20 ; TEMPORIN, S21 ; TURATTO, M22 ; WHEELER, J. C17 ; TAUBENBERGER, S3 ; SMARTT, S. J1 ; ARKHAROV, A. A4 ; BÄRNBANTNER, O5 ; BARWIG, H5 ; BENETTI, S2
[1] Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 INN, United Kingdom
[2] INAF Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
[3] Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei München, Germany
[4] Central Astronomical Observatory of Pulkovo, 196140 St Petersburg, Russian Federation
[5] Universitats-Sternwarte Miinchen, Scheinerstr. I, 81679 München, Germany
[6] Great Shefford Observatory, Phlox Cottage, Wantage Road, Great Shefford RG17 7DA, United Kingdom
[7] INAF Osservatorio Astronomico di Collurania, via M. Maggini, 64100 Teramo, Italy
[8] Dipartmento ofAstronomia, Universitd di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
[9] Spitzer Science Center, California Institute of Technology, 1200 East California Blvd, Pasadena, CA 91125, United States
[10] Astronomical Institute of St Petersburg University, St Petersburg, Petrodvorets, Universitetsky pr. 28, 198504 St Petersburg, Russian Federation
[11] Astroclub Radebeul, Auf den Ebenbergen 10a, 01445 Radebeul, Germany
[12] Fundación Galileo Galilei-INAF, Telescopio Nazionale Galileo, 38700 Santa Cruz de la Palma, Tenerife, Spain
[13] Department of Physics, Florida State University, 315 Keen Building, Tallahassee, FL 32306-4350, United States
[14] Gretelbaumbachstr. 31, 97424 Schweinfurt, Germany
[15] Isaac Newton Institute of Chile, St Petersburg Branch, United States
[16] Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
[17] Department of Astronomy and McDonald Observatory, The University of Texas at Austin, 1 University Station, C1400 Austin, Texas 78712-0259, United States
[18] INAF Osservatorio Astronomico di Roma, Via di Frascati 33, 00040 Monte Porzio Catone, Italy
[19] Department of Physics, Rochester Institute of Technology, 85 Lomb Memorial Drive, Rochester, NY 14623-5603, United States
[20] Dipartimento di Fisica, Universitd di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Roma, Italy
[21] CEA Sacly, DSM/IRFU/SAp, AIM -Unité Mixte de Recherche CEA -CNRS -Université Pans Diderot -UMR715, 91191 Gif-sur-Yvette, France
[22] INAF Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy - Source
Monthly notices of the Royal Astronomical Society (Print). 2009, Vol 394, Num 4, pp 2266-2282, 17 p ; ref : 1 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Wiley-Blackwell, Malden, MA
- Publication country
- United States
- Document type
- Article
- Language
- Russian
- Author keyword
- galaxies: individual: M51 supernovae: general supernovae: individual: SN 1997D supernovae: individual: SN 1999br supernovae: individual: SN 2003Z supernovae: individual: SN 2005cs
- Keyword (fr)
- Courbe lumière Effondrement Galaxies spirales Luminosité Modèle Observation UV Observation optique Spectre IR proche Supernova Vitesse expansion
- Keyword (en)
- Light curves Collapse Spiral galaxies Luminosity Models Ultraviolet observation Optical observation Near infrared spectrum Supernovae Expansion velocity
- Keyword (es)
- Desmoronamiento Modelo Observación UV Observación óptica Espectro IR próximo Velocidad expansión
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 21331116
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1111/j.1365-2966.2009.14505.x 
https://dx.doi.org/10.1111/j.1365-2966.2009.14505.x
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