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Infrared photometry of giants in the globular cluster NGC 4833

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dc.contributor.author Seal, P
dc.date.accessioned 2006-04-10T08:44:53Z
dc.date.available 2006-04-10T08:44:53Z
dc.date.issued 1986-09
dc.identifier.citation BASI, Vol. 14, No. 3, pp. 168-174 en
dc.identifier.uri http://hdl.handle.net/2248/915
dc.description.abstract Infrared 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 yr en
dc.format.extent 439560 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of Indian en
dc.subject Globular cluster en
dc.subject Infrared photometry en
dc.subject Red giant stars en
dc.title Infrared photometry of giants in the globular cluster NGC 4833 en
dc.type Article en


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