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W134: A New Pre-Main Sequence Double-Lined Spectroscopic Binary
We report the discovery that the pre-main sequence star Walker 134 in the young cluster NGC 2264 is a double-lined spectroscopic binary.
Document ID
20210004673
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
hdl:2014/36296
Authors
Stapelfeldt, Karl R.
Padgett, Deborah L.
Date Acquired
January 1, 1993
Publication Date
January 1, 1993
Publication Information
Publisher:
UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
Walker
134
NGC
2264
spectroscopic
binary
G
stars
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