UCAC3 152-281185 , the SIMBAD biblio

UCAC3 152-281185 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.08.06CEST08:55:39


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Title First 3 Authors
2017A&A...599A..70J viz 61       D     X         2 194 10 Binaries among low-mass stars in nearby young moving groups. JANSON M., DURKAN S., HIPPLER S., et al.
2017MNRAS.469..579B 17       D               1 127 5 A WISE-based search for debris discs amongst M dwarfs in nearby, young, moving groups. BINKS A.S. and JEFFRIES R.D.
2016A&A...589A..26B 43         O X         1 49 6 A non-uniform distribution of the nearest brown dwarfs. BIHAIN G. and SCHOLZ R.-D.
2016A&A...591A.118S viz 17       D               1 31386 40 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2014ApJ...788...81M viz 16       D               9 351 66 BANYAN. III. Radial velocity, rotation, and X-ray emission of low-mass star candidates in nearby young kinematic groups. MALO L., ARTIGAU E., DOYON R., et al.
2014ApJ...792...37M 16       D               1 96 69 BANYAN. IV. Fundamental parameters of low-mass star candidates in nearby young stellar kinematic Groups–Isochronal age determination using magnetic evolutionary models. MALO L., DOYON R., FEIDEN G.A., et al.
2013ApJ...762...88M viz 16       D               1 488 223 Bayesian analysis to identify new star candidates in nearby young stellar kinematic groups. MALO L., DOYON R., LAFRENIERE D., et al.
2012ApJ...753..156K viz 96       D       C       3 484 190 Further defining spectral type "Y" and exploring the low-mass end of the field brown dwarf mass function. KIRKPATRICK J.D., GELINO C.R., CUSHING M.C., et al.
2009ApJS..184..138H viz 16       D               1 20771 30 XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. HAAKONSEN C.B. and RUTLEDGE R.E.
2006AJ....132..866R viz 15       D               1080 83 Identification of new M dwarfs in the solar neighborhood. RIAZ B., GIZIS J.E. and HARVIN J.

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2020.08.06-08:55:39

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