Slesnick, Catherine L. and Carpenter, John M. and Hillenbrand, Lynne A. and Mamajek, Eric E. (2006) A Distributed Population of Low-Mass Pre-Main-Sequence Stars near the Taurus Molecular Clouds. Astronomical Journal, 132 (6). pp. 2665-2674. ISSN 0004-6256 http://resolver.caltech.edu/CaltechAUTHORS:20110809-111207808
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We present a drift-scan survey covering a ~5° × 50° region toward the southern portion of the Taurus-Auriga molecular cloud. Data taken in the B,R,I filters with the Quest-2 camera on the Palomar 48 inch (1.2 m) Samuel Oschin Telescope were combined with Two Micron All Sky Survey near-infrared photometry to select candidate young stars. Follow-up optical spectroscopy of 190 candidates led to the identification of 42 new low-mass pre-main-sequence stars with spectral types M4-M8, of which approximately half exhibit surface gravity signatures similar to known Taurus stars, while the other half exhibit surface gravity signatures similar to members of the somewhat older Upper Scorpius, TW Hya, and β Pic associations. The pre-main-sequence stars are spread over ~35°, and many are located well outside of previously explored regions. From assessment of the spatial and proper-motion distributions, we argue that the new pre-main-sequence stars identified far from the clouds cannot have originated from the vicinity of the 1-2 Myr old subclusters that contain the bulk of the identified Taurus members but instead represent a newly identified area of recent star formation near the clouds.
|Additional Information:||© 2006 The American Astronomical Society. Received 2006 August 3; accepted 2006 August 31. Published 2006 November 7. The authors are appreciative of the Quest-2 collaboration, including David Rabinowitz, Anne Bauer, and Jonathan Jerke, for observing and processing the photometric drift-scan data. We would like to thank Ashish Mahabal and Eilat Glikman for many discussions concerning the systematics and calibration of the Quest-2 data. We thank Lee Hartmann for his insights and suggestions, which improved the quality of this manuscript. We are grateful to assistance from the entire Palomar staff, in particular Jean Mueller, Karl Dunscombe, and Dipali. This manuscript has made use of data from the Two Micron All Sky Survey.|
|Subject Keywords:||open clusters and associations: individual (Taurus); stars: low-mass, brown dwarfs; stars: pre-main sequence|
|Official Citation:||A Distributed Population of Low-Mass Pre-Main-Sequence Stars near the Taurus Molecular Clouds Catherine L. Slesnick, John M. Carpenter, Lynne A. Hillenbrand, and Eric E. Mamajek doi: 10.1086/508937|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||09 Aug 2011 18:30|
|Last Modified:||26 Dec 2012 13:28|
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