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High-velocity features in the spectra of the Type Ia supernova SN 1999ee: a property of the explosion or evidence of circumstellar interaction?

Author
MAZZALI, P. A1 2 3 4 ; BENETTI, S5 ; STEHIE, M4 6 ; BRANCH, D7 ; DENG, J2 3 ; MAEDA, K2 3 ; NOMOTO, K2 3 ; HAMUY, M8
[1] INAF-Osservatorio Astronomico, Via Tiepolo, 11, 34131 Trieste, Italy
[2] Department of Astronomy, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
[3] Research Centre for the Early Universe, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
[4] Max-Planck Institut für Astrophysik, Karl-Schwarzschildstr 1, 85748 Garching, Germany
[5] INAF-Osservatorio Astronomico, vicolo dell'Osservatorio, 5, 35122 Padova, Italy
[6] Universitäts-Sternwarte München, Scheinerstr, 1, 81679 München, Germany
[7] Astronomy Department, Univ. of Oklahoma, Norman, OK, United States
[8] Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101-1292, United States
Source

Monthly Notices of the Royal Astronomical Society. 2005, Vol 357, Num 1, pp 200-206, 7 p ; ref : 24 ref

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
supernovae: general supernovae: individual: SN 1999ee
Keyword (fr)
Abondance Combustion nucléaire Diffusion électron Elargissement raie Perturbation Supernova type I Triplet
Keyword (en)
Abundance Burnup Electron scattering Line broadening Disturbances Type I supernova Triplets
Keyword (es)
Difusión electrón Supernova tipo I
Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16459168

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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