SPY - the ESO Supernovae type Ia Progenitor survey

Details SPY - the ESO Supernovae type Ia Progenitor survey SPY - the ESO Supernovae type Ia Progenitor survey

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003msngr.112...25n&link_type=abstract

The Messenger (ISSN 0722-6691), No. 112, p. 25 - 30 (June 2003)

Physics

77

Spy (Eso Sn Ia Progenitor Survey), Supernovae, Surveys

Scientific paper

Supernovae (SNe) mark the violent termination of a star's life in an explosion. They are classified according to their light curve as type I or II, with the type I SNe producing very similar light curves, while the SNe type II are more diverse. Spectroscopic observations reveal the presence of hydrogen in SNe type II, while no hydrogen lines are detectable in SNe type I. According to their spectral appearance the type I class can be further subdivided into Ia, Ib, and Ic.

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