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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4089
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dc.contributor.authorParthasarathy, M-
dc.date.accessioned2008-12-16T15:13:45Z-
dc.date.available2008-12-16T15:13:45Z-
dc.date.issued1978-
dc.identifier.citationThe 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 - 28en
dc.identifier.urihttp://hdl.handle.net/2248/4089-
dc.descriptionOpen Access-
dc.description.abstractThe 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 starsen
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.ispartofseriesInternational Astronomical Union Symposium, No. 80-
dc.relation.urihttp://adsabs.harvard.edu/abs/1978IAUS...80...25Pen
dc.rights©International Astronomical Union-
dc.subjectB Starsen
dc.subjectM Starsen
dc.subjectMagellanic Cloudsen
dc.subjectO Starsen
dc.subjectGalactic Structureen
dc.subjectSpectrum Analysisen
dc.subjectStellar Spectraen
dc.titleRed and blue stars in the direction of the Large Magellanic Clouden
dc.typeArticleen
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