Please use this identifier to cite or link to this item:
Title: Probable binary open star clusters in the Galaxy.
Authors: Subramaniam, A
Gorti, U
Sagar, R
Bhatt, H. C
Keywords: Star clusters;Binary clusters;Galaxy;Galaxy clustering;Clustering of Galaxies
Issue Date: Oct-1995
Publisher: EDP Science
Citation: A&A, Vol. 302, No. 1, pp. 86 - 89
Abstract: The existence of double/binary clusters in the Magellanic Clouds is fairly well established, whereas only one such pair, h + χ Persei, is known in the Galaxy. From the catalogues of open clusters of the Galaxy, we have identified 18 probable pairs of clusters (with known distances), with spatial separations less than 20pc. The tidal disruption timescales for these pairs, due to Galactic differential rotation are calculated, using cluster data where available or by assuming typical values. In some cases, these timescales are larger than the average open cluster lifetime, =~10^8^yr. About 8% of open clusters appear to be members of binary systems, and hence binary cluster systems may not be very uncommon in the Galaxy.
ISSN: 0004-6361
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Subramaniam.pdf580.63 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.