Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-17T15:17:23.115Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric and spectroscopic study of candidate Be stars in the Magellanic Clouds

Published online by Cambridge University Press:  12 July 2011

Paul KT ,
Annapurni Subramaniam ,
Blesson Mathew ,
Ronald E. Mennickent  and
Beatriz Sabogal
Paul KT
Affiliation:
Christ University, Bangalore
Annapurni Subramaniam
Affiliation:
Indian institute of Astrophysics, Bangalore
Blesson Mathew
Affiliation:
Indian institute of Astrophysics, Bangalore
Ronald E. Mennickent
Affiliation:
University of Concepcion, Chile
Beatriz Sabogal
Affiliation:
Universidad de los Andes, Colombia
Rights & Permissions [Opens in a new window]

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.

Mennickent et al. (2002) presented a catalogue of 1056 Be star candidates in the Small Magellanic cloud (SMC) by studying light curve variation using OGLE II data base. They classified these Be star candidates of the SMC in four categories: Type 1 stars showing outbursts (139 stars); Type 2 stars showing sudden luminosity jumps (154 stars); Type 3 stars showing periodic or near periodic variations (78 stars); Type 4 stars showing light curves similar to Galactic Be stars (658 stars). They suggested that Type 4 could be Be stars. On the other hand, they suggested that Type-3 stars may not be linked to the Be star phenomenon at all.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 294 - 295
Copyright
Copyright © International Astronomical Union 2011

References

Mennickent, R. E., Pietrzyński, G., Gieren, W., & Szewczyk, O. 2002, A&A 393, 887Google Scholar
Sabogal, B. E., Mennickent, R. E., Pietrzyński, G., & Gieren, W. 2005, MNRAS 361, 1055CrossRefGoogle Scholar