L 277-66 , the SIMBAD biblio

L 277-66 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST00:36:01


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Title First 3 Authors
1955LFT...C......0L 13       D               1 1843 3 Luyten's Five Tenths. LUYTEN W.J.
1979LHS...C......0L viz 14       D               4461 ~ A catalogue of stars with proper motions exceeding 0".5 annually (2nd edition). LUYTEN W.J.
2002AJ....124.1190L viz 217 96 New high proper motion stars from the Digitized Sky Survey. I. Northern stars with 0".5 yr–1<µ<2".0 yr–1 at low galactic latitudes. LEPINE S., SHARA M.M. and RICH R.M.
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.
2005A&A...435..363D viz 146 60 Southern infrared proper motion survey. I. Discovery of new high proper motion stars from first full hemisphere scan. DEACON N.R., HAMBLY N.C. and COOKE J.A.
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.
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.
2017AJ....153...14W viz 16       D               3 161 11 The solar neighborhood XXXVIII. Results from the CTIO/SMARTS 0.9M: trigonometric parallaxes for 151 nearby M dwarf systems. WINTERS J.G., SEVRINSKY R.A., JAO W.-C., 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.
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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