L 140-289 , the SIMBAD biblio

L 140-289 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST13:11:25

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1955LFT...C......0L 13       D               1 1843 3 Luyten's Five Tenths. LUYTEN W.J.
1978Ap&SS..59...35A 696 17 Kinematical and orbital properties for selected southern high-velocity stars. AUGENSEN H.J. and BUSCOMBE W.
1979LHS...C......0L viz 14       D               4461 ~ A catalogue of stars with proper motions exceeding 0".5 annually (2nd edition). LUYTEN W.J.
1997A&AS..124..437R viz 493 2 Astrometric positions of stars with high proper motions in the Southern Hemisphere. ROUSSEAU J.-M. and PERIE J.-P.
2002ApJS..141..187B viz 4465 67 Revised coordinates and proper motions of the stars in the Luyten half-second catalog. BAKOS G.A., SAHU K.C. and NEMETH P.
2010AJ....140..897R 168       D     X         5 69 48 The solar neighborhood. XXII. Parallax results from the CTIOPI 0.9 M program: trigonometric parallaxes of 64 nearby systems with 0".5 ≤µ≤ 1".0 /yr (SLOWMO sample). RIEDEL A.R., SUBASAVAGE J.P., FINCH C.T., et al.
2014AJ....147...21J 16       D               1 26 18 The solar neighborhood. XXXI. Discovery of an unusual red+white dwarf binary at ∼25 pc via astrometry and UV imaging. JAO W.-C., HENRY T.J., SUBASAVAGE J.P., et al.
2014MNRAS.443.2561G viz 16       D               1 2978 190 Trumpeting M dwarfs with CONCH-SHELL: a catalogue of nearby cool host-stars for habitable exoplanets and life. GAIDOS E., MANN A.W., LEPINE S., et al.
2015AJ....149....5W viz 16       D               1 1773 104 The solar neighborhood. XXXV. Distances to 1404 M dwarf systems within 25 pc in the southern sky. WINTERS J.G., HAMBLY N.C., JAO W.-C., et al.
2015AJ....150....6H viz 16       D               1 276 16 The solar neighborhood. XXXVI. The long-term photometric variability of nearby red dwarfs in the VRI optical bands. HOSEY A.D., HENRY T.J., JAO W.-C., et al.
2016ApJ...817..112S viz 16       D               1 20551 25 A proper motion survey using the first sky pass of NEOWISE-reactivation data. SCHNEIDER A.C., GRECO J., CUSHING M.C., et al.
2016ApJS..224...36K viz 16       D               1 45305 70 The AllWISE motion survey, part 2. KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.C., et al.
2018AJ....156..217N viz 16       D               1 580 80 New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars. NEWTON E.R., MONDRIK N., IRWIN J., et al.
1995yCat.1098....0L viz 14       D               1 52092 ~ New Luyten Catalogue of stars with proper motions larger than two tenths of an arcsecond (NLTT). LUYTEN W.J.
2019ApJ...874L...8K viz 17       D               1 1816 6 TESS Habitable Zone star Catalog. KALTENEGGER L., PEPPER J., STASSUN K., et al.
2020ApJS..247...11R viz 17       D               1 46227 22 Radial velocity photon limits for the dwarf stars of spectral classes F-M. REINERS A. and ZECHMEISTER M.
2020AJ....160..215V viz 17       D               1 605 16 The solar neighborhood. XLVI. Revealing new M dwarf binaries and their orbital architectures. VRIJMOET E.H., HENRY T.J., JAO W.-C., et al.
2020ApJ...905..107M viz 17       D               1 135 39 Flare rates, rotation periods, and spectroscopic activity indicators of a volume-complete sample of mid- to late-M dwarfs within 15 pc. MEDINA A.A., WINTERS J.G., IRWIN J.M., et al.
2021AJ....161...63W viz 17       D               1 574 22 The volume-complete sample of M dwarfs with masses 0.1 <= M/M☉ <= 0.3 within 15 parsecs. WINTERS J.G., CHARBONNEAU D., HENRY T.J., et al.
2021AJ....161..233K viz 17       D               1 6504 ~ Around which stars can TESS detect Earth-like planets? The Revised TESS Habitable Zone Catalog. KALTENEGGER L., PEPPER J., CHRISTODOULOU P.M., et al.
2021A&A...649A...6G viz 17       D               1 89188 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.

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