Project Details
Description
ARE HARD X-RAY SYMBIOTICS PROGENITORS OF TYPE IA SUPERNOVAE? Symbiotic stars are interacting binaries in which a white dwarf (WD) accretes from the wind of a red giant. Their X-ray emission is typically very soft. Recently, however, 4 symbiotics have been
| Status | Finished |
|---|---|
| Effective start/end date | 1/31/08 → 1/30/10 |
Funding
- National Aeronautics and Space Administration: US$25,320.00
ASJC Scopus Subject Areas
- Radiation
- Space and Planetary Science
- Astronomy and Astrophysics
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