A shell ejection model for optical light variations in Be stars: Application to Be/X ray binaries

Details A shell ejection model for optical light variations in Be stars: Application to Be/X ray binaries A shell ejection model for optical light variations in Be stars: Application to Be/X ray binaries

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..521d&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 521-523 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Light Curve, Stellar Mass Ejection, Stellar Models, X Ray Astronomy, X Ray Binaries, B Stars, Stellar Luminosity, Stellar Magnitude, Variability, Variable Stars

Scientific paper

A model for light variations in Be stars where changes in the mass loss rate occur in the form of shell ejections is presented. Optical variations of the order of tenths of magnitude on a timescale ranging from days to several weeks are predicted by the model. A correlation between Be/X ray binaries optical light variations and X ray activity is investigated. An application to the Be/X ray binary A0535+26/HDE 245770 is presented.

Affiliated with

Also associated with

No associations

Rating

A shell ejection model for optical light variations in Be stars: Application to Be/X ray binaries 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 A shell ejection model for optical light variations in Be stars: Application to Be/X ray binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A shell ejection model for optical light variations in Be stars: Application to Be/X ray binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1614747