Constraining type Ia supernovae progenitors from three years of supernova legacy survey data
While it is generally accepted that Type Ia supernovae are the result of the explosion of a carbon-oxygen white dwarf accreting mass in a binary system, the details of their genesis still elude us, and the nature of the binary companion is uncertain. Kasen points out that the presence of a non-degen...
| Hlavní autoři: | , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Médium: | Journal article |
| Jazyk: | English |
| Vydáno: |
2011
|