Luminous Supersoft X-Ray Sources as Progenitors of Type IA Supernovae

Details Luminous Supersoft X-Ray Sources as Progenitors of Type IA Supernovae Luminous Supersoft X-Ray Sources as Progenitors of Type IA Supernovae

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996sao..reptr....d&link_type=abstract

Technical Report, Harvard-Smithsonian Center for Astrophysics Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Supernovae, X Ray Sources, White Dwarf Stars, Observation, Hydrogen, Combustion

Scientific paper

In some luminous supersoft X-ray sources, hydrogen accretes onto the surface of a white dwarf at rates more-or-less compatible with steady nuclear burning. The white dwarfs in these systems therefore have a good chance to grow in mass. Here we review what is known about the rate of Type la supernovae that may be associated with SSSS. Observable consequences of the conjecture that SSSs can be progenitors of Type Ia supernovae are also discussed.

Affiliated with

Also associated with

No associations

Rating

Luminous Supersoft X-Ray Sources as Progenitors of Type IA Supernovae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Luminous Supersoft X-Ray Sources as Progenitors of Type IA Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminous Supersoft X-Ray Sources as Progenitors of Type IA Supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1129879