StKM 1-2018A , the SIMBAD biblio

StKM 1-2018A , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:00:46


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Title First 3 Authors
2007ApJ...654..558D 57 37 Discovery of nine new companions to nearby young M stars with the Altair AO system. DAEMGEN S., SIEGLER N., REID I.N., et al.
2009ApJ...699..649S viz 15       D               1 187 162 Identifying the young low-mass stars within 25 pc. I. Spectroscopic observations. SHKOLNIK E., LIU M.C. and REID I.N.
2012ApJ...758...56S viz 15       D               1 196 148 Identifying the young low-mass stars within 25 pc. II. Distances, kinematics, and group membership. SHKOLNIK E.L., ANGLADA-ESCUDE G., LIU M.C., et al.
2014A&A...567A..52K viz 15       D   O           1 157 18 Reliable probabilistic determination of membership in stellar kinematic groups in the young disk. KLUTSCH A., FREIRE FERRERO R., GUILLOUT P., et al.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al.
2024A&A...684A...3Y 18       D               1 104 ~ Radio emission as a stellar activity indicator. YIU T.W.H., VEDANTHAM H.K., CALLINGHAM J.R., et al.
2024A&A...686A.164W viz 18       D               1 1620 ~ Magnetic activity of radio stars based on TESS and LAMOST surveys. WANG Y., ZHANG L., SU T., et al.
2024PASA...41...84D viz 18       D               1 863 ~ The Sydney Radio Star Catalogue: Properties of radio stars at megahertz to gigahertz frequencies. DRIESSEN L.N., PRITCHARD J., MURPHY T., et al.
2024A&A...692A.206C viz 18       D               1 2241 ~ CARMENES input catalogue of M dwarfs VIII. Kinematics in the solar neighbourhood. CORTES-CONTRERAS M., CABALLERO J.A., MONTES D., et al.

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