{ "id": "2409.15579", "version": "v1", "published": "2024-09-23T22:28:05.000Z", "updated": "2024-09-23T22:28:05.000Z", "title": "Spectroscopic Observations of the Galex Nearby Young Star Survey Sample. 1. Nearby Moving Group Candidates", "authors": [ "Navya Nagananda", "Laura Vican", "Ben Zuckerman", "David Rodriguez", "Alexander Binks", "Joel Kastner" ], "comment": "The paper is accepted by the Open Journal of Astrophysics", "categories": [ "astro-ph.SR", "astro-ph.EP", "astro-ph.GA" ], "abstract": "The GALEX Nearby Young Star Search (GALNYSS) yielded the identification of more than 2000 late-type stars that, based on their ultraviolet and infrared colors and pre-Gaia proper motions, are potentially of age < 200 Myr and lie within ~120 pc of Earth. We present the results of a campaign of medium- and high-resolution optical spectroscopy of 471 GALNYSS stars aimed at confirming their youth and their potential membership in nearby young stellar moving groups. We present radial velocity (RV), Li absorption, and H-$\\alpha$ emission measurements for these spectroscopically observed GALNYSS stars, and assess their Li absorption and optical emission-line properties and infrared excesses. Our RV measurements are combined with literature and Gaia DR3 RV measurements and Gaia DR3 astrometry and photometry to obtain the spatiokinematics and color-magnitude positions of GALNYSS stars. We use these results to assess membership in the TW Hya, Tuc-Hor, Carina, Columba, and Argus Associations and the $\\beta$-PMG and AB Dor moving groups. We have identified 132 stars as candidate members of these seven groups; roughly half of these candidates are newly identified on the basis of data presented here. At least one-third of the 132 candidates are spectroscopic and/or photometric binaries and/or have comoving (visual) binary companions in Gaia DR3. The contingent of young, low-mass stars in the solar vicinity we identify here should provide excellent subjects for future direct imaging exoplanet surveys and studies of the early evolution of low-mass stars and their planetary progeny.", "revisions": [ { "version": "v1", "updated": "2024-09-23T22:28:05.000Z" } ], "analyses": { "keywords": [ "galex nearby young star survey", "nearby young star survey sample", "nearby moving group candidates" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }