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Supernovae interacting with a circumstellar medium: New observations with X-shooter

✍ Scribed by A. Pastorello; S. Benetti; F. Bufano; E. Kankare; S. Mattila; M. Turatto; G. Cupani


Book ID
102756167
Publisher
John Wiley and Sons
Year
2011
Tongue
English
Weight
500 KB
Volume
332
Category
Article
ISSN
0004-6337

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✦ Synopsis


Abstract

In this article we present new data of a sample of core‐collapse supernovae showing unequivocal evidences of interaction between their ejecta and pre‐existing circumstellar matter (CSM). This CSM was produced by the progenitor star through major mass loss episodes during the final stages of its life. The study of the properties of the SN ejecta and the circumstellar environment are crucial to unveil the nature of the progenitors producing interacting supernovae. In this context, the instrumental combination Very Large Telescope (VLT) plus X‐shooter provides spectra covering simultaneously the optical and near‐infrared domains, and with adequate resolution to constrain the main properties of the supernova and its environment, including its chemical composition, the ejection velocity and the distribution of the emitting gas (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)


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