A new method to identify nearby, young, low-mass stars

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Abstract

We describe a new method to identify young, late-type stars within ∼150 pc of the Earth that employs visual or near-infrared (NIR) data and the GALEX GR4/5 database. For spectral types later than K5, we demonstrate that the ratio of GALEX near-ultraviolet to visual and NIR emission is larger for stars with ages between 10 and 100 Myr than for older, main-sequence stars. A search in regions of the sky encompassing the TW Hya and Scorpius-Centaurus Associations has returned 54 high-quality candidates for follow up. Spectroscopic observations of 24 of these M1-M5 objects reveal Li 6708 Å absorption in at least 17 systems. Because GALEX surveys have covered a significant fraction of the sky, this methodology should prove valuable for future young star studies. © 2011. The American Astronomical Society.

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Rodriguez, D. R., Bessell, M. S., Zuckerman, B., & Kastner, J. H. (2011). A new method to identify nearby, young, low-mass stars. Astrophysical Journal, 727(2). https://doi.org/10.1088/0004-637X/727/2/62

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