V* KT Lib , the SIMBAD biblio

V* KT Lib , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST09:37:09


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Title First 3 Authors
1991ApJS...76.1001P viz 1762 52 Photoelectric UBV photometry of stars selected in the HK objective-prism survey. PRESTON G.W., SHECTMAN S.A. and BEERS T.C.
1994AJ....108..538P viz 365 142 The space density and kinematics of blue metal-poor main sequence stars near the solar circle. PRESTON G.W., BEERS T.C. and SHECTMAN S.A.
1999AJ....117.2329W viz 1125 45 Spectroscopy of hot stars in the galactic halo. III. Analysis of a large sample of field horizontal-branch and other A-type stars. WILHELM R., BEERS T.C., SOMMER-LARSEN J., et al.
1999AJ....118.3006P 6 11 Pulsating blue metal-poor stars. PRESTON G.W. and LANDOLT A.U.
2000AJ....120.1014P 94 203 What are these blue metal-poor stars? PRESTON G.W. and SNEDEN C.
2002A&A...391.1039K viz 67 11 The determination of Teff for metal-poor A-type stars using V and 2MASS J, H and K magnitudes. KINMAN T. and CASTELLI F.
2006ApJ...636L.129J 21 8 Discovery of an SX Phoenicis type pulsating component in the Algol-type semidetached eclipsing binary QU Sagittae in M71. JEON Y.-B., KIM S.-L., LEE M.G., et al.
2006IBVS.5721....1K viz 1754 36 The 78th name-list of variable stars. KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al.
2007ApJS..168..277B viz 15       D               1 1525 8 A catalog of candidate field horizontal-branch and A-type stars. III. A 2MASS-cleaned version. BEERS T.C., ALMEIDA T., ROSSI S., et al.
2010A&A...515A..39F viz 38           X         1 7 11 The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign. II. Evidence of a binary - possibly triple - system. FAUVAUD S., SAREYAN J.-P., RIBAS I., et al.
2017A&A...598A..54H viz 16       D               1 80 ~ Something borrowed, something blue: The nature of blue metal-poor stars inferred from their colours and chemical abundances. HANSEN C.J., JOFRE P., KOCH A., et al.
2017MNRAS.466.1290N viz 41           X         1 66 14 Metal-rich SX Phe stars in the Kepler field. NEMEC J.M., BALONA L.A., MURPHY S.J., et al.

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