G 262-22 , the SIMBAD biblio

G 262-22 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST14:50:26

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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
1976Obs....96..233W 68 T                   1 2 0 G262-21/
22, a common-proper-motion binary system consisting of two subluminous stars. 		WEGNER G.
1979ApJ...233..226L 84 109 New results from a survey of faint proper-motion stars: a probable deficiency of very low luminosity degenerates. LIEBERT J., DAHN C.C., GRESHAM M., et al.
1984VilOB..68....3B 286 8 Catalogue of metal-deficient F-M stars. Part 1. Stars classified spectroscopically. Supplement 1. BARTKEVICIUS A.
1987AJ.....93..116C 864 159 A survey of proper-motion stars. I. UBV photometry and radial velocities. CARNEY B.W. and LATHAM D.W.
1988AJ.....95.1843L 947 203 A survey of proper-motion stars. III. Reddenings, distances and metallicities. LAIRD J.B., CARNEY B.W. and LATHAM D.W.
1992AJ....104.1144R 161 51 Halo common proper motion stars: subdwarf distance scale, halo binary fraction, and UBVRI colors. RYAN S.G.
1994AJ....107.2240C viz 1436 327 A survey of proper motion stars. XII. An expanded sample. CARNEY B.W., LATHAM D.W., LAIRD J.B., et al.
1994AJ....108.2338H viz 297 62 Photographic astrometry of binary and proper-motion stars. VIII. HEINTZ W.D.
2005AJ....129.1483L viz 63380 364 A catalog of northern stars with annual proper motions larger than 0.15" (LSPM-NORTH catalog). LEPINE S. and SHARA M.M.
2011A&A...536A..50P 15       D               1 45 25 Prediction of astrometric microlensing events during the Gaia mission. PROFT S., DEMLEITNER M. and WAMBSGANSS J.
2014ApJ...790..159M 1 48 138 The end of the MACHO era, revisited: new limits on MACHO masses from halo wide binaries. MONROY-RODRIGUEZ M.A. and ALLEN C.
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.

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