Light curve solutions of eclipsing binaries in SMC

dc.contributor.author	Ivanov, V. P
dc.contributor.author	Kjurkchieva, D. P
dc.contributor.author	Srinivasa Rao, M
dc.date.accessioned	2011-01-13T10:19:17Z
dc.date.available	2011-01-13T10:19:17Z
dc.date.issued	2010-09
dc.identifier.citation	BASI, Vol. 38, No. 2&3, pp. 83-92	en
dc.identifier.uri	http://hdl.handle.net/2248/5298
dc.description.abstract	We propose a procedure for light-curve solutions of eclipsing binary stars in the Small Magellanic Cloud (SMC) for which photometric data have been obtained in the framework of the OGLE project. We also present a way of determining the global stellar parameters on the basis of the obtained solutions, some empirical relations as well as the distance to the SMC. Several examples illustrate this procedure.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://www.ncra.tifr.res.in/~basi/10JuneSep/Abstracts/380832010.htm	en
dc.rights	© Astronomical Society of India	en
dc.subject	Stars: binaries	en
dc.subject	Eclipsing - stars	en
dc.subject	Fundamental parameters - stars	en
dc.subject	General - galaxies: individual: SMC	en
dc.title	Light curve solutions of eclipsing binaries in SMC	en
dc.type	Article	en