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A Wolf-Rayet Cluster in IC 4662

Published online by Cambridge University Press:  03 August 2017

O.-G. Richter  and
M. R. Rosa
O.-G. Richter
Affiliation:
1) Space Telescope Science Institute, Baltimore, MD 21218, U.S.A. ∗ Affiliated to the Astrophysics Division of the Space Science Department of E.S.A.
M. R. Rosa
Affiliation:
2) The Space Telescope European Coordinating Facility, European Southern Observatory, Garching, F.R.G. ∗ Affiliated to the Astrophysics Division of the Space Science Department of E.S.A.

Abstract

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An imaging and spectroscopic survey for WR stars in IC 4662 revealed the presence of a cluster consisting of a mix of about 10 WN 7-8 and WC 5 stars plus the equivalent of some 5 OV stars at a projected distance of about 100 pc from the cluster core of the bright central H ii complex.

Type
Session VIII. Inventory and Distribution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 653 - 654
Copyright
Copyright © Kluwer 1991