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X-ray sources in regions of star formation. III - Naked T Tauri stars associated with the Taurus-Auriga complexGround-based and IRAS optical and IR spectroscopic and photometric observations are reported for 90 stars in or near 59 Einstein Observatory X-ray error circles in the Tau-Aur region. The data are presented in extensive tables and sample spectra and characterized in detail, with particular attention to 28 newly discovered 'naked' T Tau stars, which are shown to be normal stars with no significant IR or UV excess and ages of 1-40 Myr. These stars are found to outnumber normal T Tau stars by a factor of 10 in an area near the Tau-Aur dark clouds, and it is argued that their evolution toward the ZAMS is typical for low-mass stars. The implications of this finding for the time scales of circumstellar-disk dissipation and planet formation are discussed.
Document ID
19880057922
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Walter, Frederick M.
(Colorado Univ. Boulder, CO, United States)
Brown, A.
(Colorado, University Boulder, United States)
Mathieu, R. D.
(Colorado Univ. Boulder, CO, United States)
Myers, P. C.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Vrba, F. J.
(U.S. Naval Observatory Flagstaff, AZ, United States)
Date Acquired
August 13, 2013
Publication Date
July 1, 1988
Publication Information
Publication: Astronomical Journal
Volume: 96
ISSN: 0004-6256
Subject Category
Astrophysics
Accession Number
88A45149
Funding Number(s)
CONTRACT_GRANT: NAG8-508
CONTRACT_GRANT: NAS5-28731
CONTRACT_GRANT: NAG5-429
CONTRACT_GRANT: NGL-06-003-057
Distribution Limits
Public
Copyright
Other

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