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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/915
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dc.contributor.authorSeal, P-
dc.date.accessioned2006-04-10T08:44:53Z-
dc.date.available2006-04-10T08:44:53Z-
dc.date.issued1986-09-
dc.identifier.citationBASI, Vol. 14, No. 3, pp. 168-174en
dc.identifier.urihttp://hdl.handle.net/2248/915-
dc.description.abstractInfrared broad band JHK photometry is presented for 21 red giants in the metal-poor globular cluster NGC 4833. The color magnitude and color-color correlations are discussed. Bolometric luminosities are calculated from apparent K magnitudes by using bolometric corrections for giants. A comparison with Yale isochrones gives the most likely age of this cluster to be about 12 x 10 to the 9th yren
dc.format.extent439560 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectGlobular clusteren
dc.subjectInfrared photometryen
dc.subjectRed giant starsen
dc.titleInfrared photometry of giants in the globular cluster NGC 4833en
dc.typeArticleen
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