Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-13T13:12:15.812Z Has data issue: false hasContentIssue false
  • English
  • Français

Correlation Between Spectrum Characteristics and Photometric Behaviour of Be Stars

Published online by Cambridge University Press:  14 August 2015

G. A. Ponomareva
G. A. Ponomareva*
Affiliation:
Sternberg Astronomical Institute - Moscow

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Based upon a sample of 140 B0-A0 emission-line stars contained in “A Photographic Atlas of Be stars” statistical relationships between variable stars and Be stars are examined. It is found that 44 % of all the stars of the sample show some kind of photometric variations. The stars with narrow metallic absorption lines display relatively more intense photometric activity. Proceeding from this conclusion, the photometric variability of two stars HD 50138 and HD 193182 can be predicted.

Type
I. Photometry
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 65 - 67
Copyright
Copyright © Reidel 1982 

References

Blanco, V.M., Demers, S.; Douglass, C.G., Fitzgerald, M.P. 1968, Publ. U.S. Naval Obs., 2-d series, 21 Google Scholar
Ferrer, L., Jaschek, C. 1971, Publ. Astron. Soc. Pacific 83, 346 CrossRefGoogle Scholar
Hubert-Delplace, A.M., Hubert, H., 1979 “Un Atlas des Etoiles Be” Observatoire de Paris-Meudon and Observatoire de Haute-Provence Google Scholar
Jaschek, M., Hubert-Delplace, A.M., Hubert, H., Jaschek, C. 1980, Astron. and Astrophys. Suppl. Ser. 42, 103 Google Scholar