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Discovery of five pre-main-sequence binaries in TaurusThe progress of an infrared K band lunar occultation search for binaries among premain-sequence stars is reported. From the fall of 1986 to the fall of 1989, 13 objects have been observed, all in the Taurus star-forming region. Five new binaries have been discovered: DF Tau, DI Tau, FS Tau (Haro 6-5) A, FV Tau (Haro 6-8), and FW Tau, with projected separations ranging from 0.01 to 0.57 arcsec. Including results reported previously, a total of 31 objects, 21 in Taurus and 10 in Ophiuchus, have been surveyed and nine double systems have been found. The detected binary frequency (0.29) seems consistent with that of the solar-type main-sequence field stars.
Document ID
19900052195
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Chen, W. P.
(State Univ. of New York Stony Brook, NY, United States)
Simon, M.
(New York, State University Stony Brook, United States)
Longmore, A. J.
(Royal Observatory Edingburgh, United Kingdom)
Howell, R. R.
(State Univ. of New York Stony Brook, NY, United States)
Benson, J. A.
(Wyoming, University Laramie, United States)
Date Acquired
August 14, 2013
Publication Date
July 1, 1990
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 357
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
90A39250
Funding Number(s)
CONTRACT_GRANT: NAGW-1276
Distribution Limits
Public
Copyright
Other

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