Finding Supernova Ia Progenitors with the Chandra X-ray Observatory

Details Finding Supernova Ia Progenitors with the Chandra X-ray Observatory Finding Supernova Ia Progenitors with the Chandra X-ray Observatory

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1314..264n&link_type=abstract

INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink's 65th Birthday. AIP Conference Proceedings, Volume 1314, p

Other

Supernovae, Brightness, X-Ray Binary Stars, White Dwarfs, Accretion Disks, Supernovae, Luminosity And Mass Functions, X-Ray Binaries, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Accretion And Accretion Disks

Scientific paper

We examine pre-supernova Chandra images to find X-ray luminosities of type Ia supernova progenitors. At present, we have one possible direct detection and upper limits for the X-ray luminosities of a number of other supernova progenitors. The method has also yielded a possible detection of a X-ray binary Wolf-Rayet system as the progenitor of a type Ib supernova.

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