Consistent estimates of \mathsf⁵⁶Ni yields for type Ia supernovae

2006/09/17 by Maximilian Stritzinger, M. Stritzinger, Paolo Mazzali +5 · 5 citations
Mathematics · Physics and Astronomy · #Astrophysics #Combinatorics #Cosmology and Gravitation Theories #Gamma-ray bursts and supernovae #Geology #Mathematics #Nuclear physics research studies #Physics #Supernova #Type (biology) #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065514

Accepted for publication in A&A, constructive comments welcomed

arxiv created 2006/09/17 · openalex publication_date 2006/09/26 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims.We present mass estimates for seventeen well-observed type Ia supernovae determined by two independent methods.

Citations

• Secondary Maximum in the Near‐Infrared Light Curves of Type Ia Supernovae
• Optical and Infrared Photometry of the Unusual Type Ia Supernova 2000cx
• Determination of the Hubble Constant Using a Two‐Parameter Luminosity Correction for Type Ia Supernovae
• On the evolution of rapidly rotating massive white dwarfs towards supernovae or collapses
• Photometric observations of the Type Ia SN 2002er in UGC 10743
• Final Results from theHubble Space TelescopeKey Project to Measure the Hubble Constant
• Type Ia Supernova Explosion Models

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• Photometric observations of the supernova 2009nr
• Type Ia supernova diversity: white dwarf central density as a secondary parameter in three-dimensional delayed detonation models
• The underluminous Type Ia supernova 2005bl and the class of objects similar to SN 1991bg★