The inner zone of binary-star accretion disks

Details The inner zone of binary-star accretion disks The inner zone of binary-star accretion disks

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..134s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Mar. 1978, p. 134-137.) Soviet Astronomy Letters, vol. 4, Mar.-Apr. 1978, p. 71-73.

Astronomy and Astrophysics

Astronomy

Binary Stars, Interstellar Gas, Stellar Mass Accretion, Stellar Models, Disks (Shapes), Scattering Cross Sections, Stellar Coronas, Stellar Gravitation, Stellar Motions, Thomson Scattering, Velocity Distribution

Scientific paper

A model is worked out for the inner zone of an accretion disk, allowing
for the existence of a vertical velocity component for the gas. The
temperature in the central plane of the disk is found to be higher than
in the standard theory, and it depends on the accretion rate. Some of
the gas in the inner zone is shed, producing a corona around the disk.

Affiliated with

Also associated with

No associations

Rating

The inner zone of binary-star accretion disks 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 The inner zone of binary-star accretion disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The inner zone of binary-star accretion disks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1381024