AO535+26 and the structure of the outflowing gas from Be stars

Details AO535+26 and the structure of the outflowing gas from Be stars AO535+26 and the structure of the outflowing gas from Be stars

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989chjss...9q.161m&link_type=abstract

(Chinese Journal of Space Science, vol. 9, no. 3, 1989, p. 161-167) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13

Astronomy and Astrophysics

Astrophysics

B Stars, Stellar Mass Ejection, Stellar Winds, X Ray Binaries, Disks, Flow Velocity, Light Curve, Luminosity, Neutron Stars

Scientific paper

The paper proposes a hybrid model, a gas disk plus a slowly accelerating
stellar wind, for the gas outflow from the Be star in transient hard
X-ray binaries. The velocity structure in the outflow is presented, the
variation of the X-luminosity is calculated, and many observed features
of AO535+26 are explained.

Affiliated with

Also associated with

No associations

Rating

AO535+26 and the structure of the outflowing gas from Be stars 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 AO535+26 and the structure of the outflowing gas from Be stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and AO535+26 and the structure of the outflowing gas from Be stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-764498