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- W3100484716 endingPage "60" @default.
- W3100484716 startingPage "60" @default.
- W3100484716 abstract "Young stars in the solar neighborhood serve as nearby probes of stellar evolution and represent promising targets to directly image self-luminous giant planets. We have carried out an all-sky search for late-type ($approx$K7$-$M5) stars within 100 pc selected primarily on the basis of activity indicators from $GALEX$ and $ROSAT$. Approximately two thousand active and potentially young stars are identified, over 600 of which we have followed up with low-resolution optical spectroscopy and over 1000 with diffraction-limited imaging using Robo-AO at the Palomar 1.5-m telescope. Strong lithium is present in 58 stars, implying ages spanning $approx$10$-$200 Myr. Most of these lithium-rich stars are new or previously known members of young moving groups including TWA, $beta$ Pic, Tuc-Hor, Carina, Columba, Argus, AB Dor, Upper Centaurus Lupus, and Lower Centaurus Crux; the rest appear to be young low-mass stars without connections to established kinematic groups. Over 200 close binaries are identified down to 0.2$''$ $-$ the vast majority of which are new $-$ and will be valuable for dynamical mass measurements of young stars with continued orbit monitoring in the future." @default.
- W3100484716 created "2020-11-23" @default.
- W3100484716 creator A5003301860 @default.
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- W3100484716 creator A5055884799 @default.
- W3100484716 creator A5059756978 @default.
- W3100484716 creator A5067120075 @default.
- W3100484716 date "2019-05-24" @default.
- W3100484716 modified "2023-10-10" @default.
- W3100484716 title "The Elusive Majority of Young Moving Groups. I. Young Binaries and Lithium-rich Stars in the Solar Neighborhood" @default.
- W3100484716 cites W1495614800 @default.
- W3100484716 cites W1575766262 @default.
- W3100484716 cites W1656352035 @default.
- W3100484716 cites W1860427147 @default.
- W3100484716 cites W1883299030 @default.
- W3100484716 cites W1965097857 @default.
- W3100484716 cites W1965696912 @default.
- W3100484716 cites W1965864262 @default.
- W3100484716 cites W1967409881 @default.
- W3100484716 cites W1968233503 @default.
- W3100484716 cites W1979161213 @default.
- W3100484716 cites W1991502431 @default.
- W3100484716 cites W1993999573 @default.
- W3100484716 cites W1996255849 @default.
- W3100484716 cites W1996537612 @default.
- W3100484716 cites W1997870235 @default.
- W3100484716 cites W1997910565 @default.
- W3100484716 cites W1999208145 @default.
- W3100484716 cites W2001705480 @default.
- W3100484716 cites W2003917323 @default.
- W3100484716 cites W2006978661 @default.
- W3100484716 cites W2008204335 @default.
- W3100484716 cites W2009254894 @default.
- W3100484716 cites W2011945362 @default.
- W3100484716 cites W2016333448 @default.
- W3100484716 cites W2017062400 @default.
- W3100484716 cites W2021537216 @default.
- W3100484716 cites W2021657959 @default.
- W3100484716 cites W2024059141 @default.
- W3100484716 cites W2026840775 @default.
- W3100484716 cites W2028424239 @default.
- W3100484716 cites W2028569725 @default.
- W3100484716 cites W2030264067 @default.
- W3100484716 cites W2030663701 @default.
- W3100484716 cites W2035753114 @default.
- W3100484716 cites W2038416916 @default.
- W3100484716 cites W2042037826 @default.
- W3100484716 cites W2042084648 @default.
- W3100484716 cites W2042114541 @default.
- W3100484716 cites W2047534186 @default.
- W3100484716 cites W2052548770 @default.
- W3100484716 cites W2052937506 @default.
- W3100484716 cites W2059439802 @default.
- W3100484716 cites W2064846308 @default.
- W3100484716 cites W2068012642 @default.
- W3100484716 cites W2068325771 @default.
- W3100484716 cites W2074559645 @default.
- W3100484716 cites W2074648364 @default.
- W3100484716 cites W2078112089 @default.
- W3100484716 cites W2078503872 @default.
- W3100484716 cites W2079581806 @default.
- W3100484716 cites W2084132830 @default.
- W3100484716 cites W2086521183 @default.
- W3100484716 cites W2087569457 @default.
- W3100484716 cites W2088330484 @default.
- W3100484716 cites W2089598844 @default.
- W3100484716 cites W2090231561 @default.
- W3100484716 cites W2091939413 @default.
- W3100484716 cites W2106723742 @default.
- W3100484716 cites W2106873657 @default.
- W3100484716 cites W2107745751 @default.
- W3100484716 cites W2114892626 @default.
- W3100484716 cites W2130197607 @default.
- W3100484716 cites W2133493128 @default.
- W3100484716 cites W2135415545 @default.
- W3100484716 cites W2142220522 @default.
- W3100484716 cites W2149716536 @default.
- W3100484716 cites W2159697822 @default.
- W3100484716 cites W2167180582 @default.
- W3100484716 cites W2172169673 @default.
- W3100484716 cites W2195588120 @default.
- W3100484716 cites W2213126889 @default.
- W3100484716 cites W2238392768 @default.
- W3100484716 cites W2259286564 @default.
- W3100484716 cites W2261573924 @default.
- W3100484716 cites W2395172868 @default.
- W3100484716 cites W2395288238 @default.
- W3100484716 cites W2538512269 @default.
- W3100484716 cites W2622776717 @default.
- W3100484716 cites W2636932883 @default.
- W3100484716 cites W2751042743 @default.
- W3100484716 cites W2785063374 @default.