Intracluster extinction in young open star clusters

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