dc.contributor.author |
Mohan, V |
|
dc.contributor.author |
Sagar, R |
|
dc.date.accessioned |
2006-04-11T08:30:11Z |
|
dc.date.available |
2006-04-11T08:30:11Z |
|
dc.date.issued |
1988-12 |
|
dc.identifier.citation |
BASI, Vol. 16, No. 4, pp. 159-182 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/947 |
|
dc.description.abstract |
Photographic photometry of about 900 stars down to V = 17 mag has been carried out in the region of the open cluster NGC 2301. The cluster region seems to be severely contaminated by field stars. Statistical criteria yield only 96 + or - 17 cluster members. Stars fainter than about 15 mag are found to be absent among cluster members. Star counts indicate a diameter of about 20 arcmin. The data suggest mass segregation in the cluster |
en |
dc.format.extent |
1563664 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of Indian |
en |
dc.subject |
Open cluster |
en |
dc.subject |
Photographic photometry |
en |
dc.subject |
Star counts |
en |
dc.title |
Field star contamination in open star cluster NGC 2301 |
en |
dc.type |
Article |
en |