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

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..279n&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 279-282 (2010).

Other

Brightness, Astronomical Observatories, X-Ray Binary Stars, Supernovae, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Observatories And Site Testing, X-Ray Binaries, Supernovae

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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