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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5597

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DC Field	Value	Language
dc.contributor.author	Paul, K. T	-
dc.contributor.author	Subramaniam, A	-
dc.contributor.author	Mathew, B	-
dc.contributor.author	Mennickent, R. E	-
dc.contributor.author	Sabogal, B	-
dc.date.accessioned	2011-09-30T09:19:26Z	-
dc.date.available	2011-09-30T09:19:26Z	-
dc.date.issued	2011-07	-
dc.identifier.citation	Proceedings of the International Astronomical Union Symposium, Vol. 272, 294-295	en
dc.identifier.uri	http://hdl.handle.net/2248/5597	-
dc.description	Open Access	en
dc.description.abstract	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.	en
dc.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.uri	http://dx.doi.org/10.1017/S1743921311010635	en
dc.rights	© Cambridge University Press	en
dc.title	Photometric and spectroscopic study of candidate Be stars in the Magellanic Clouds	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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