X-ray binaries in globular clusters

Details X-ray binaries in globular clusters X-ray binaries in globular clusters

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988iraj...18..152c&link_type=abstract

Irish Astronomical Journal (ISSN 0021-1052), vol. 18, March 1988, p. 152-157.

Astronomy and Astrophysics

Astronomy

Milky Way Galaxy, Neutron Stars, Stellar Mass Accretion, White Dwarf Stars, X Ray Binaries, Black Holes (Astronomy), Stellar Mass Ejection, X Ray Astronomy, X Ray Sources

Scientific paper

The bright galactic X-ray sources are known to derive their energy from
the accretion of material onto a compact, degenerate object - either a
white dwarf, neutron star or black hole. This infalling gas must itself
originate from a nearby mass-losing companion, and thus most of the
bright X-ray sources in the Galaxy must be binary systems.

Affiliated with

Also associated with

No associations

Rating

X-ray binaries in globular clusters 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 binaries in globular clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray binaries in globular clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674765