SNeIa: on the binary progenitors and expected statistics

1996/09/10 by P. Ruiz-Lapuente, P. Ruiz‐Lapuente, Ruiz-Lapuente, P. +4
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9609078

ps file, 26 pages, incl. 6 figs. and 2 tables. To appear in "Thermonuclear Supernovae", ed. P. Ruiz-Lapuente, R. Canal, & J. Isern (Kluwer Acad. Publ.)

arxiv created 1996/09/10 · openalex publication_date 1996/09/10 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

A review of type Ia supernovae (SNe Ia) statistics as expected from the different scenarios and explosion models so far suggested is presented.

Related

• Progenitors of Supernovae Type Ia
• The search for progenitor models of type Ia supernovae
• Binary population synthesis and SNIa rates
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• Type Ia supernovae