Red and blue stars in the direction of the Large Magellanic Cloud

dc.contributor.author	Parthasarathy, M
dc.date.accessioned	2008-12-16T15:13:45Z
dc.date.available	2008-12-16T15:13:45Z
dc.date.issued	1978
dc.identifier.citation	The HR diagram - The 100th anniversary of Henry Norris Russell; Proceedings of the Symposium, Washington, D.C., November 2 - 5, 1977. (A79-14326 03-89) Dordrecht, D. Reidel Publishing Co., 1978, pp. 25 - 28	en
dc.identifier.uri	http://hdl.handle.net/2248/4089
dc.description	Open Access
dc.description.abstract	The Large Magellanic Cloud has been surveyed on ultralow dispersion (10,000 A/mm) plates taken with the 102-centimeter reflector at Kavalur. Many new red and blue stars were found. The LMC bar was found to have a strong component of red stars and a very weak component of faint OB stars. In general the regions other than the bar contain very luminous OB stars, faint OB stars and a few very red stars. The 30 Doradus complex is rich in luminous red and blue stars	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.ispartofseries	International Astronomical Union Symposium, No. 80
dc.relation.uri	http://adsabs.harvard.edu/abs/1978IAUS...80...25P	en
dc.rights	©International Astronomical Union
dc.subject	B Stars	en
dc.subject	M Stars	en
dc.subject	Magellanic Clouds	en
dc.subject	O Stars	en
dc.subject	Galactic Structure	en
dc.subject	Spectrum Analysis	en
dc.subject	Stellar Spectra	en
dc.title	Red and blue stars in the direction of the Large Magellanic Cloud	en
dc.type	Article	en