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

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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

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