A study of Be stars variability

Details A study of Be stars variability A study of Be stars variability

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98...19d&link_type=abstract

In: Be stars; Proceedings of the Symposium, Munich, West Germany, April 6-10, 1981. (A83-10301 01-90) Dordrecht, D. Reidel Publi

Computer Science

22

B Stars, Stellar Spectra, Variable Stars, Balmer Series, Infrared Spectra, Light Curve, Visible Spectrum

Scientific paper

Variations of Balmer emission line strength for Be stars are compared to simultaneously measured photometric light-curves in the visual and infrared regions of the spectrum. Three different types of correlations between photometric and spectrometric variations are described. Variable intensity of continuous recombination radiation from ionized hydrogen in the circumstellar envelope is shown to be a major source of light variations for Be stars.

Affiliated with

Also associated with

No associations

Rating

A study of Be stars variability 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 study of Be stars variability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A study of Be stars variability will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-841878