PM J10019+6651 , the SIMBAD biblio

PM J10019+6651 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST12:12:21


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Title First 3 Authors
2003A&A...406..535Z viz 15       D               1 10290 80 The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources. ZICKGRAF F.-J., ENGELS D., HAGEN H.-J., et al.
2011AJ....142..138L viz 15       D               1 8897 232 An all-sky catalog of bright M dwarfs. LEPINE S. and GAIDOS E.
2012AJ....143...80S viz 15       D               2 231 76 Cool young stars in the northern hemisphere: β Pictoris and AB Doradus moving group candidates. SCHLIEDER J.E., LEPINE S. and SIMON M.
2012AJ....144..109S 15       D               2 42 41 Likely members of the β Pictoris and AB Doradus moving groups in the north. SCHLIEDER J.E., LEPINE S. and SIMON M.
2013MNRAS.435.2161F viz 16       D               1 8411 18 A catalogue of bright (K < 9) M dwarfs. FRITH J., PINFIELD D.J., JONES H.R.A., et al.
2015ApJ...798...41A viz 16       D               1 802 19 The near-ultraviolet luminosity function of young, early M-type dwarf stars. ANSDELL M., GAIDOS E., MANN A.W., et al.
2016MNRAS.455.3345B 177       D       C F     5 68 17 Spectroscopic confirmation of M-dwarf candidate members of the Beta Pictoris and AB Doradus Moving Groups. BINKS A.S. and JEFFRIES R.D.
2017A&A...600A..83M viz 260       D   O X C       6 150 9 The β Pictoris association: Catalog of photometric rotational periods of low-mass members and candidate members. MESSINA S., MILLWARD M., BUCCINO A., et al.
2017A&A...607A...3M 16       D   O           2 125 3 The β Pictoris association low-mass members: Membership assessment, rotation period distribution, and dependence on multiplicity. MESSINA S., LANZAFAME A.C., MALO L., et al.
2019ApJ...877...60B viz 17       D               2 658 26 The elusive majority of young moving groups. I. Young binaries and lithium-rich stars in the solar neighborhood. BOWLER B.P., HINKLEY S., ZIEGLER C., et al.

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