A model for repeatedly bursting X-ray sources

Details A model for repeatedly bursting X-ray sources A model for repeatedly bursting X-ray sources

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210l..19h&link_type=abstract

Astrophysical Journal, vol. 210, Nov. 15, 1976, pt. 2, p. L19-L22.

Astronomy and Astrophysics

Astronomy

17

Astronomical Models, Binary Stars, Neutron Stars, White Dwarf Stars, X Ray Sources, Interstellar Matter, Magnetoacoustic Waves, Variable Stars, X Ray Astronomy, X Ray Stars

Scientific paper

A model for bursting X-ray sources given in 1972 is elaborated and
extended. Application to the recently discovered sources 3U 1820-30 and
MXB 1730-335 shows that the former is likely to be a neutron star in a
dense interstellar cloud, while the latter source appears to be a white
dwarf in a binary system.

Affiliated with

Also associated with

No associations

Rating

A model for repeatedly bursting 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 A model for repeatedly bursting X-ray sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A model for repeatedly bursting X-ray sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1725203