A near-infrared photometric study of the young Orion nebula star cluster NGC 1976

Qian, Z. Y. ; Sagar, R. (1994) A near-infrared photometric study of the young Orion nebula star cluster NGC 1976 Monthly Notices of the Royal Astronomical Society, 266 (1). pp. 114-122. ISSN 0035-8711

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Official URL: http://adsabs.harvard.edu/abs/1994MNRAS.266..114Q

Abstract

We have measured the JHK magnitudes of 47 stars in the region of the extremely young Orion nebula star cluster NGC 1976. These, in combination with the existing near-infrared and optical data, are used to study the intracluster extinction law. This indicates an anomalous distribution of intracluster grains in the vicinity of many stars causing less extinction in the U, B, R and I passbands than that obtained from the colour excess E(V-J) using a normal interstellar extinction law. This implies a small shift in the grain size distribution towards larger than normal sized particles in these regions.

Item Type:Article
Source:Copyright of this article belongs to John Wiley and Sons.
Keywords:Dust; Extinction; ISM: General; Open Clusters and Associations: Individual: NGC 1976; Infrared: General
ID Code:65942
Deposited On:20 Oct 2011 06:18
Last Modified:20 Oct 2011 06:18

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