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LP 912-32 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.28CET19:48:02 |
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 |
---|---|---|---|---|---|---|---|---|---|
1979LHS...C......0L | 14 | D | 4461 | ~ | A catalogue of stars with proper motions exceeding 0".5 annually (2nd edition). | LUYTEN W.J. | |||
1985AJ.....90...74E | 98 | 28 | Systematic search for members of the Hyades supercluster. VI. The lower main sequence. | EGGEN O.J. | |||||
1987AJ.....93..379E | 992 | 38 | Catalog of proper-motion stars. III. Stars brighter than visual magnitude 15.1, south of declination +30, and with annual proper motion between 0.5 and 0.7 arcsec. | EGGEN O.J. | |||||
1990PASP..102..166E | 111 | 15 | K- and M-type dwarf stars within 25 parsecs of the Sun. I. The age-chromospheric activity relation from H-alpha equivalent widths. | EGGEN O.J. | |||||
1991NSC3..C......0G | 1352 | ~ | Preliminary Version of the third catalogue of nearby stars. | GLIESE W. and JAHREISS H. | |||||
1995AJ....109..797K | 67 | 207 | The solar neighborhood. II. The first list of dwarfs with spectral types of M7 and cooler. | KIRKPATRICK J.D., HENRY T.J. and SIMONS D.A. | |||||
1995AJ....110.1838R | 1848 | 572 | The Palomar/MSU nearby-star spectroscopic survey. I. The northern M dwarfs-band strengths and kinematics. | REID I.N., HAWLEY S.L. and GIZIS J.E. | |||||
1996AJ....112.2799H | 2161 | 422 | The Palomar/MSU nearby star spectroscopic survey. II. The southern M dwarfs and investigations of magnetic activity. | HAWLEY S.L., GIZIS J.E. and REID I.N. | |||||
2001ApJS..133..119R | 542 | 38 | Calan-ESO proper-motion catalog. | RUIZ M.T., WISCHNJEWSKY M., ROJO P.M., et al. | |||||
2002AJ....123.2806R | 524 | 94 | Meeting the cool neighbors. I. Nearby stars in the NLTT catalogue: defining the sample. | REID I.N. and CRUZ K.L. | |||||
2002ApJS..141..187B | 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. | |||||
2003ApJ...582.1011S | 35377 | 223 | Improved astrometry and photometry for the Luyten catalog. II. Faint stars and the revised catalog. | SALIM S. and GOULD A. | |||||
2006AJ....132.1234C | 55 | 77 | The solar neighborhood. XVI. Parallaxes from CTIOPI: final results from the 1.5m telescope program. | COSTA E., MENDEZ R.A., JAO W.-C., et al. | |||||
2007A&A...468..163D | 15 | D | 1 | 7019 | 33 | Southern infrared proper motion survey. II. A sample of low mass stars with µ≥0.1"/yr. | DEACON N.R. and HAMBLY N.C. | ||
2010PASP..122..885S | 15 | D | 1 | 3982 | 28 | Accurate coordinates and 2MASS cross identifications for (almost) all Gliese catalog star. | STAUFFER J., TANNER A.M., BRYDEN G., et al. | ||
2011ApJS..197...19K | 15 | D | 1 | 575 | 330 | The first hundred brown dwarfs discovered by the Wide-field Infrared Survey Explorer (WISE). | KIRKPATRICK J.D., CUSHING M.C., GELINO C.R., et al. | ||
2014AJ....148..119F | 16 | D | 1 | 1765 | 12 | UCAC4 nearby star survey: a search for our stellar neighbors. | FINCH C.T., ZACHARIAS N., SUBASAVAGE J.P., et al. | ||
2015AJ....149....5W | 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. | ||
2016ApJ...817..112S | 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. | ||
2017ApJ...834...85N | 16 | D | 1 | 2207 | 217 | The Hα emission of nearby M dwarfs and its relation to stellar rotation. | NEWTON E.R., IRWIN J., CHARBONNEAU D., et al. | ||
2018AJ....156..217N | 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 | 14 | D | 1 | 52092 | ~ | New Luyten Catalogue of stars with proper motions larger than two tenths of an arcsecond (NLTT). | LUYTEN W.J. |