Computer Science
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98...53d&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
11
B Stars, Balmer Series, Data Correlation, Interstellar Extinction, Stellar Envelopes, Stellar Spectra, Continuous Spectra, Parameterization, Stellar Luminosity, Variable Stars
Scientific paper
The separation of the effects of interstellar reddening from effects due to the presence of the envelope which is necessary for the interpretation of the continuous spectrum of Be stars, is avoided through the use of the two types of correlations presented. In the first of these, parameters not affected by interstellar reddening, such as the Balmer jump and decrement, are used. In the second one, the parameters used may be affected by the interstellar extinction, but comparisons are restricted to values corresponding to the same variable Be star, at different epochs, with different amounts of emission.
Briot Danielle
Divan Lucienne
Zorec Jean
No associations
LandOfFree
Correlations between BCD parameters of the continuous spectrum and the Balmer decrement of 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 Correlations between BCD parameters of the continuous spectrum and the Balmer decrement of Be stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Correlations between BCD parameters of the continuous spectrum and the Balmer decrement of Be stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-841898