Thermonuclear flashes in a degenerate neutron-star envelope

Details Thermonuclear flashes in a degenerate neutron-star envelope Thermonuclear flashes in a degenerate neutron-star envelope

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5...34t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Jan. 1979, p. 34-38.) Soviet Astronomy Letters, vol. 5, Jan.-Feb. 1979, p. 20-22. Tr

Astronomy and Astrophysics

Astronomy

1

Degeneration, Flare Stars, Neutron Stars, Stellar Envelopes, Thermonuclear Reactions, X Ray Sources, Gas Density, Stellar Evolution, Stellar Mass Accretion, Stellar Temperature

Scientific paper

The thermonuclear model of X-ray burst sources is invoked to analyze the conditions whereby flash instability can occur in the accretion envelope of a neutron star. Flares lasting from a few seconds to several days and spaced from hours to hundreds of years apart can be understood in terms of the thermonuclear mechanism. A single flare would release 10 to the 39th to 10 to the 45th erg of energy.

Affiliated with

Also associated with

No associations

Rating

Thermonuclear flashes in a degenerate neutron-star envelope 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 Thermonuclear flashes in a degenerate neutron-star envelope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermonuclear flashes in a degenerate neutron-star envelope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-830791