The radial structure of hot one-temperature accretion flows with advection.

Details The radial structure of hot one-temperature accretion flows with advection. The radial structure of hot one-temperature accretion flows with advection.

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..239l&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 3, p. 239 - 248

Astronomy and Astrophysics

Astrophysics

Accretion: Structure, Accretion: Advection

Scientific paper

Considering nonthermal e±-pair production, this paper is focused on the radial structure of hot one-temperature accretion flows with advection under the condition of a small viscous parameter (α = 0.1) and low mass-accretion rates. Self-similar relations of hot flow with advection have been adopted. The authors have used a scheme, in which the two regions of accretion flow are calculated separately and then joined together. Some typical features of hot flow with advection have been confirmed, and several new results obtained.

Affiliated with

Also associated with

No associations

Rating

The radial structure of hot one-temperature accretion flows with advection. 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 radial structure of hot one-temperature accretion flows with advection., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The radial structure of hot one-temperature accretion flows with advection. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1184190