X-Ray Emission from White Dwarfs in Close Binary Systems

Details X-Ray Emission from White Dwarfs in Close Binary Systems X-Ray Emission from White Dwarfs in Close Binary Systems

Mar 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973pthph..49..776h&link_type=abstract

Progress of Theoretical Physics, Vol. 49, No. 3, pp. 776-789

Physics

61

Scientific paper

The generation of X-ray sources in close binary systems is studied. It
is proposed that one of the stars is a white dwarf and it is accreting
material from its companion. The entire treatment applies to the
sphericaly symmetric and the stationary case. The model of this type
accounts qualitatively for the observed nature of SCO X-1.

Affiliated with

Also associated with

No associations

Rating

X-Ray Emission from White Dwarfs in Close Binary Systems 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 X-Ray Emission from White Dwarfs in Close Binary Systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-Ray Emission from White Dwarfs in Close Binary Systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1639613