SNe Ia: On the Binary Progenitors and Expected Statistics

作者: P. Ruiz-Lapuente , R. Canal , A. Burkert

DOI: 10.1007/978-94-011-5710-0_14

关键词:

摘要: Type la supernovae (SNe Ia) are explosions of C+O WDs triggered by the accretion material from a companion. After many years SN research, we fairly certain nature exploding object, but very little is still known about companion star. In fact, it has been long noticed that does not leave its imprint on explosion in way which could allow us to identify progenitor system. It hoped near future various observational tests discussed along this conference will shed light into identification issue.

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