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The embedded cluster or association Trumpler 37 in IC 1396: a search for evolutionary constraints
Article first published online: 20 MAR 2012
DOI: 10.1111/j.1365-2966.2012.20541.x
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Issue
Monthly Notices of the Royal Astronomical Society
Volume 421, Issue 4, pages 3206–3216, April 2012
Additional Information
How to Cite
Saurin, T. A., Bica, E. and Bonatto, C. (2012), The embedded cluster or association Trumpler 37 in IC 1396: a search for evolutionary constraints. Monthly Notices of the Royal Astronomical Society, 421: 3206–3216. doi: 10.1111/j.1365-2966.2012.20541.x
Publication History
- Issue published online: 10 APR 2012
- Article first published online: 20 MAR 2012
- Accepted 2012 January 12. Received 2012 January 11; in original form 2011 September 15
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Keywords:
- open clusters and associations: individual: Trumpler 37;
- open clusters and associations: individual: Teutsch 74
ABSTRACT
It is currently widely accepted that open star clusters and stellar associations result from the evolution of embedded star clusters. Parameters such star formation efficiency, time-scale of gas removal and velocity dispersion can be determinants of their future as bound or unbound systems. Finding objects at an intermediate evolution state can provide constraints to model the embedded cluster evolution. In the H ii region IC 1396, Trumpler 37 is an extended young cluster that presents characteristics of an association. We employed the Two Micron All Sky Survey (2MASS) photometry for analysing its structure and stellar content, and determining its astrophysical parameters. We also analysed 11 bright-rimmed clouds in IC 1396 in order to search for young infrared star clusters, and the background open star cluster Teutsch 74, to verify whether it has any contribution to the observed stellar density profile of Trumpler 37. The derived parameters and comparison with template objects from other studies lead us to conclude that Trumpler 37, rather than as a star cluster, will probably emerge from its molecular cloud as an OB association.