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New weak-line T Tauri stars in Taurus-Auriga (Li+ 1998)
New weak-line T Tauri stars in Taurus-Auriga (Li+ 1998)
Apr 1998
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adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..41320173l&link_type=abstract
VizieR On-line Data Catalog: J/A+AS/132/173. Originally published in: 1998A&AS..132..173L
Computer Science
Stars: Pre-Main Sequence, X-Ray Sources
Scientific paper
We present results of an extensive search for weak-line T Tauri stars (WTTS) in the outskirts of the Taurus-Auriga molecular cloud on the basis of the ROSAT All-Sky Survey Bright Source Catalog (Cat. ). Our surveyed region extends from 2h 40m to 5h 40m in right ascension and from 10deg to 40deg in declination, with the central part of Taurus-Auriga(4h<α<5h, 15deg<δ<34deg), accomplished by Wichmann et al. (1996, Cat. ), excluded. Within a sky coverage of about 10$3$ square degrees, 219 X-ray sources fullfill the criteria for selecting program sources suggested by Neuhauser et al. (1995A&A...295L...5N) and 164 of these X-ray sources were found to have at least one optical counterpart with E magnitude brighter than 16. Low-resolution spectroscopic observation has been carried out in order to discard early type stars and galaxies from the sample, additional intermediate-resolution spectra of a sub-sample of 156 late type optical counterparts were obtained for spectral classification and for the calculation of the equivalent width of Hα emission and LiI line absorption at 6707Å. Excluding 2 previously identified WTTS, a total of 75 new candidate WTTS and one possible classical T Tauri star have been discovered in our study. The majority of the newly found Li-rich optical counterparts are believed to b e PMS stars rather than ZAMS stars as those of the Pleiades. (4 data files).
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