Stellar Accretion and X-ray Emission

Details Stellar Accretion and X-ray Emission Stellar Accretion and X-ray Emission

Jul 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.215..464c&link_type=abstract

Nature, Volume 215, Issue 5100, pp. 464-466 (1967).

Computer Science

58

Scientific paper

Shklovsky has suggested that the Scorpius X-ray source is a binary pair and that the X-radiation arises from the collision of material from a giant star with a neutron star. The theoretical complications of such a model are now found not to match actual measurements and it is suggested that the bremsstrahlung effect occurs between a giant star and a white dwarf.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1211920