Please use this identifier to cite or link to this item:
Full metadata record
DC FieldValueLanguage
dc.contributor.authorPaul, K. T-
dc.contributor.authorSubramaniam, A-
dc.contributor.authorMathew, B-
dc.contributor.authorMennickent, R. E-
dc.contributor.authorSabogal, B-
dc.identifier.citationProceedings of the International Astronomical Union Symposium, Vol. 272, 294-295en
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.publisherCambridge University Pressen
dc.rights© Cambridge University Pressen
dc.titlePhotometric and spectroscopic study of candidate Be stars in the Magellanic Cloudsen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Photometric and spectroscopic study of candidate Be stars.pdfOpen Access189.06 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.