NAME KA 2 , the SIMBAD biblio

NAME KA 2 , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST18:50:47


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Title First 3 Authors
1985AJ.....90.2244H 65 40 CH stars as galaxy halo tracers. HARTWICK F.D.A. and COWLEY A.P.
1990VilOB..85....3S 153 27 Catalogue of CH and metal-deficient barium stars. SLEIVYTE J. and BARTKEVICIUS A.
1992ApJ...400..659G 50 48 Carbon star luminosity indicators. GREEN P.J., MARGON B. and ANDERSON S.F.
1994PASP..106.1134D 8 13 Positions and proper motions of dwarf carbon stars. DEUTSCH E.W.
1996BaltA...5..217B 257 21 A new version of the catalog of CH and related stars (CH95 catalog). BARTKEVICIUS A.
1998MNRAS.294....1T 90 113 The APM survey for cool carbon stars in the Galactic halo - I. TOTTEN E.J. and IRWIN M.J.
2001A&A...375..366C viz 410 121 The stellar content of the Hamburg/ESO survey. II. A large, homogeneously-selected sample of high latitude carbon stars. CHRISTLIEB N., GREEN P.J., WISOTZKI L., et al.
2001BaltA..10....1A viz 6821 114 General catalog of galactic carbon stars by C.B. Stephenson. Third edition. ALKSNIS A., BALKLAVS A., DZERVITIS U., et al.
2003ApJ...584L..95L 31 18 The discovery of two nearby carbon dwarfs. LOWRANCE P.J., KIRKPATRICK J.D., REID I.N., et al.
2007ApJS..168..128B viz 15       D               1852 38 Broadband UBVRCIC photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I. BEERS T.C., FLYNN C., ROSSI S., et al.
2007A&A...463..969M 51 8 The properties of carbon stars found in the Byurakan and the Hamburg/ESO surveys. MAURON N., GIGOYAN K.S. and KENDALL T.R.
2010MNRAS.402.1111G 625       D S   X C F     14 109 23 The CH fraction of carbon stars at high galactic latitudes. GOSWAMI A., KARINKUZHI D. and SHANTIKUMAR N.S.
2012A&A...544A..95G 39           X         1 20 9 New carbon stars found in the Digitized First Byurakan Survey. GIGOYAN K.S., RUSSEIL D., MICKAELIAN A.M., et al.
2018MNRAS.479.3873W 16       D               1 28 7 Dwarf carbon stars are likely metal-poor binaries and unlikely hosts to carbon planets. WHITEHOUSE L.J., FARIHI J., GREEN P.J., et al.

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