The evolutionary sequence of nonmassive X-ray binaries

Details The evolutionary sequence of nonmassive X-ray binaries The evolutionary sequence of nonmassive X-ray binaries

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..995a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Sept.-Oct. 1988, p. 995-1005. In Russian.

Astronomy and Astrophysics

Astronomy

Milky Way Galaxy, Stellar Evolution, Stellar Systems, X Ray Binaries, Novae, Nuclear Fusion, Star Distribution, Stellar Motions, Supernovae

Scientific paper

The following evolutionary sequence of nonmassive X-ray binaries is
substantiated: (1) weak X-ray sources with the phenomena of X-ray novae,
(2) bright stable sources, (3) bright sources with the phenomena of
bursters, and X-ray bursters. The spatial distribution of these types of
sources in the Galaxy is analyzed. Their main parameters are determined.

Affiliated with

Also associated with

No associations

Rating

The evolutionary sequence of nonmassive X-ray binaries 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 The evolutionary sequence of nonmassive X-ray binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolutionary sequence of nonmassive X-ray binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1598363