Published August 1996
| Published
Journal Article
Open
Low-Mass Stars in an Outer Field in NGC 6397
- Creators
-
Mould, Jeremy R.
- Watson, Alan M.
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Gallagher, John S., III
- Ballester, Gilda E.
- Burrows, Christopher J.
- Casertano, Stefano
- Clarke, John T.
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Crisp, David
- Griffiths, Richard E.
- Hester, J. Jeff
- Hoessel, John G.
- Holtzman, Jon A.
- Scowen, Paul A.
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Stapelfeldt, Karl R.
- Trauger, John T.
- Westphal, James A.
Chicago
Abstract
We have imaged a field 10' from the center of the globular cluster NGC 6397 in the visible and I bands with WFPC2 on the Η ST. At a level which is severely limited by counting statistics in the small area so far studied, this field is richer in dwarfs with />21.5 than the 4:6 radius parallel field discussed by Paresce and colleagues. This indicates that the dynamical process of mass segregation is occurring in the cluster.
Additional Information
© 1996 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System. Received 1996 February 29; accepted 1996 May 31. This research was carried out by the WFPC2 Investigation Definition Team for JPL and was sponsored by NASA through Contract No. NAS7-1260. J.R.M. wishes to thank Gary Da Costa for helpful discussions and the referee for useful comments.Attached Files
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Additional details
- Eprint ID
- 53680
- Resolver ID
- CaltechAUTHORS:20150114-094315944
- NASA
- NAS7-1260
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2015-01-14Created from EPrint's datestamp field
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2021-11-10Created from EPrint's last_modified field