Be/X ray sources

Details Be/X ray sources Be/X ray sources

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..437j&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 437-438 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Stellar Luminosity, Stellar Mass Accretion, Stellar Systems, X Ray Binaries, B Stars, Balmer Series, Infrared Astronomy, Stellar Envelopes, Stellar Orbits, Stellar Spectra, Variable Stars, X Ray Spectra

Scientific paper

The X-ray luminosities observed in eight Be/X-ray systems are explained.
The observed and calculated maximum X-ray luminosities for such systems
are compared assuming that the neutron stars are in equatorial orbits
and accrete from dense, slowly expanding, Be envelopes responsible for
the IR excess and Balmer emission.

Affiliated with

Also associated with

No associations

Rating

Be/X ray sources 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 Be/X ray sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Be/X ray sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1614665