SIMBAD references

2011ApJ...727...62R - Astrophys. J., 727, 62 (2011/February-1)

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

RODRIGUEZ D.R., BESSELL M.S., ZUCKERMAN B. and KASTNER J.H.

Abstract (from CDS):

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.

Abstract Copyright:

Journal keyword(s): open clusters and associations: individual (Lower Centaurus Crux, Upper Centaurus Lupus, TW Hydrae) - stars: evolution - stars: pre-main sequence - ultraviolet: stars

CDS comments: TWA 32 is 2MASS J12265135-3316124 in SIMBAD.

Simbad objects: 64

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2020.02.26-01:41:11

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