Matches in SemOpenAlex for { <https://semopenalex.org/work/W3101161669> ?p ?o ?g. }
- W3101161669 endingPage "251" @default.
- W3101161669 startingPage "241" @default.
- W3101161669 abstract "Bolometric light curves provide a valuable insight into the nature of type Ia supernovae. We present an analysis of sixteen well-observed type Ia supernovae. Constraints are placed on several global parameters concerning the progenitor system, explosion mechanism, and subsequent radiation transport. By fitting a radioactive decay energy deposition function to the quasi-exponential phase (50 to 100 days after maximum light), it is found that the ejected mass varies by at least a factor of two. This result suggests that a sub Chandrasekhar mass white dwarf could be the progenitor system of some type Ia supernovae. We find that the range in the amount of synthesized indicates a significant variation in the burning mechanism. In order to explain a factor of ten range in the observed bolometric luminosity, more detailed modeling of the explosion mechanism is required." @default.
- W3101161669 created "2020-11-23" @default.
- W3101161669 creator A5018273831 @default.
- W3101161669 creator A5049514978 @default.
- W3101161669 creator A5051144522 @default.
- W3101161669 creator A5081952162 @default.
- W3101161669 date "2006-04-01" @default.
- W3101161669 modified "2023-09-26" @default.
- W3101161669 title "Constraints on the progenitor systems of type Ia supernovae" @default.
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- W3101161669 doi "https://doi.org/10.1051/0004-6361:20053652" @default.