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Synthetic Spectra of the Type Ia SN 2002bo

Published online by Cambridge University Press:  19 September 2016

M. Stehle  and
P.A. Mazzali
M. Stehle
Affiliation:
Max-Planck-Institut für Astrophysik, P.O. Box 1317 85741 Garching, Germany;mstehle@mpa-garching.mpg.de Universitäts-Sternwarte München, Scheinerstr. 1, 81679 München, Germany
P.A. Mazzali
Affiliation:
Max-Planck-Institut für Astrophysik, P.O. Box 1317 85741 Garching, Germany;mstehle@mpa-garching.mpg.de INAF - Osservatorio Astronomico di Trieste, Via Tiepolo, 11, 34131 Trieste, Italy;mazzali@ts.astro.it

Summary

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SN 2002bo, a type Ia supernova in NGC 3190, is the first object of the European Supernova Collaboration (ESC). It was discovered on 09 March 2002 and is one of the earliest observed SNe. An almost complete set of spectra and photometry is available from 13 days before maximum B light until a few days after. An analysis using synthetic spectra is presented, focusing on the controversial issue of the reddening of SN 2002bo.

Type
Part I Supernovae: Individual
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 129 - 133
Copyright
Copyright © Springer-Verlag 2005

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