Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5597
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dc.contributor.authorPaul, K. T-
dc.contributor.authorSubramaniam, A-
dc.contributor.authorMathew, B-
dc.contributor.authorMennickent, R. E-
dc.contributor.authorSabogal, B-
dc.date.accessioned2011-09-30T09:19:26Z-
dc.date.available2011-09-30T09:19:26Z-
dc.date.issued2011-07-
dc.identifier.citationProceedings of the International Astronomical Union Symposium, Vol. 272, 294-295en
dc.identifier.urihttp://hdl.handle.net/2248/5597-
dc.descriptionOpen Accessen
dc.description.abstractMennickent 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.isoenen
dc.publisherCambridge University Pressen
dc.relation.urihttp://dx.doi.org/10.1017/S1743921311010635en
dc.rights© Cambridge University Pressen
dc.titlePhotometric and spectroscopic study of candidate Be stars in the Magellanic Cloudsen
dc.typeArticleen
Appears in Collections:IIAP Publications

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