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http://hdl.handle.net/2248/353
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Scaria, K. K | - |
dc.date.accessioned | 2005-02-09T06:37:15Z | - |
dc.date.available | 2005-02-09T06:37:15Z | - |
dc.date.issued | 1982-12 | - |
dc.identifier.citation | BASI, Vol. 10, No. 4, pp. 340 - 347 | en |
dc.identifier.uri | http://hdl.handle.net/2248/353 | - |
dc.description | Open Access | - |
dc.description.abstract | Integrated magnitudes in U, B, V, R and I bands are calculated for the globular cluseter Omega Centauri. The observed radial chaange in the integrated colour of the cluster shows that the cluster core (r<2') is redder in R - I colour and blure in U - B colour. It is argued that there is an increase in the ratio of AGB stars to the red gaints towards the centre of the cluster. | en |
dc.format.extent | 696091 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | - |
dc.publisher | Astronomical Society of India | en |
dc.subject | Integrated Brightness | en |
dc.subject | Globular Cluster | en |
dc.subject | Omega Centauri | en |
dc.title | Integrated brightness and colour of Omega Centauri | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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Integrated brightness and colour | Open Access | 679.78 kB | Adobe PDF | View/Open |
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