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 |
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dc.format.mimetype |
application/pdf |
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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 |