WIYN Open Cluster Study. XVII. Astrometry and Membership toV=21 in NGC 188
Author(s) -
I. Platais,
V. Kozhurina-Platais,
Robert D. Mathieu,
Terrence M. Girard,
W. F. van Altena
Publication year - 2003
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/379677
Subject(s) - astrometry , physics , proper motion , stars , open cluster , astrophysics , galaxy , reference frame , distortion (music) , cluster (spacecraft) , astronomy , frame (networking) , computer science , telecommunications , amplifier , optoelectronics , cmos , programming language
We present techniques for obtaining presision astrometry using oldphotographic plates from assorted large-aperture reflectors in combination withrecent CCD Mosaic Imager frames. At the core of this approach is atransformation of plate/CCD coordinates into a previously constructedastrometric reference frame around the open cluster NGC 188. Our primary resultis a new catalog of proper motions and positions for 7812 objects down to V=21in the 0.75 square degree area around NGC 188. The precision for well-measuredstars is 0.15 mas/yr for proper motions and 2 mas for positions on the systemof the Tycho-2 catalog. The sum of membership probabilities indicates that NGC188 contains 1050 stars down to V=21. Comprehensive lists of the candidate bluestragglers and red giants substantially enlarge the number of such stars knownin NGC 188. We have also obtained a small correction to the proper motions fromthe mean `motion' of background galaxies. (Abridged)Comment: 37 pages, 10 figures. Accepted for publication in The Astronomical Journa
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