Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/1555
Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Sagar, R | - |
dc.contributor.author | Qian, Z. Y | - |
dc.date.accessioned | 2007-05-09T08:30:01Z | - |
dc.date.available | 2007-05-09T08:30:01Z | - |
dc.date.issued | 1993 | - |
dc.identifier.citation | BASI, Vol. 21, pp. 565-568 | en |
dc.identifier.uri | http://hdl.handle.net/2248/1555 | - |
dc.description.abstract | An analysis of near-infrared data in combination with optical observations, indicates a normal interstellar extinction law around hot O and B stars at wavelengths greater than or = 0.9 micrometers. At shorter wavelengths, it can be either normal or anomalous depending upon the physical conditions of intracluster material. In some cases, anomaly is found to be due to a small shift in grain-size distribution towards smaller than normal sized particle, while in other regions, exactly opposite grain size distribution seems to be responsible for the anomaly. | en |
dc.format.extent | 280626 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.subject | Star clusters | en |
dc.subject | Star formation | en |
dc.title | Intracluster extinction in young open star clusters | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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Paper_15.pdf | 274.05 kB | Adobe PDF | ![]() View/Open |
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