The correlation between the spectrum characteristics and photometric behavior of Be stars

Details The correlation between the spectrum characteristics and photometric behavior of Be stars The correlation between the spectrum characteristics and photometric behavior of Be stars

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981sval....7..228p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, July 1981, p. 414-416.) Soviet Astronomy Letters, vol. 7, July-Aug. 1981, p. 228-230

Astronomy and Astrophysics

Astronomy

1

Absorption Spectra, B Stars, Spectral Correlation, Stellar Luminosity, Stellar Spectrophotometry, Variable Stars, Abundance, Metals, Star Distribution

Scientific paper

Spectroscopic properties of 140 bright Be stars surveyed by Jaschek et al. (1980) are compared against their photometric behavior. It is found that 44% of the stars in the sample are variable, with those possessing narrow metal absorption lines especially active photometrically. The normalized distribution of Be stars with respect to spectral type is presented, and it is predicted that variable brightness should develop in the Be stars HD 50138 and HD 193182, which have narrow metal absorption lines and are currently thought to be nonvariable.

Affiliated with

Also associated with

No associations

Rating

The correlation between the spectrum characteristics and photometric behavior 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 The correlation between the spectrum characteristics and photometric behavior of Be stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The correlation between the spectrum characteristics and photometric behavior of Be stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1748872