HD 156384B , the SIMBAD biblio

HD 156384B , the SIMBAD biblio (27 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST02:00:01


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Title First 3 Authors
1979VKha..190...52Z viz 334 5 Nearest stars. ZAKHOZHAJ V.A.
1980SAAOC...1..166C 594 68 VRI photometry of nearby stars. COUSINS A.W.J.
1983ApJS...53..643J 1981 18 Predicted infrared brightness of stars within 25 parsecs of the Sun. JOHNSON H.M. and WRIGHT C.D.
1985ApJS...59..197B viz 14       D               1 3393 78 G.P. Kuiper's spectral classifications of proper-motion stars. BIDELMAN W.P.
1994MNRAS.267..840H 310 26 ROSAT EUV luminosity functions of nearby late-type stars. HODGKIN S.T. and PYE J.P.
1994KFNT...10b..68Z 96 0 The masses of the nearest stars. ZAKHOZHAJ V.A.
1994KFNT...10b..74Z 128 0 Infrared sources in the neighbourhood of the Sun. ZAKHOZHAJ V.A., SHAPARENKO E.F., VASILEV V.P., et al.
1997A&AS..124...75T viz 14       D               1 1447 254 MSC - a catalogue of physical multiple stars. TOKOVININ A.A.
1999A&AS..135..319H viz 1221 244 The ROSAT all-sky survey catalogue of the nearby stars. HUENSCH M., SCHMITT J.H.M.M., STERZIK M.F., et al.
2001A&A...367..521P viz 6126 101 Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics. PASINETTI FRACASSINI L.E., PASTORI L., COVINO S., et al.
2001AJ....121.2189O viz 154 78 A coronagraphic survey for companions of stars within 8 parsecs. OPPENHEIMER B.R., GOLIMOWSKI D.A., KULKARNI S.R., et al.
2002KFNT...18f.535Z 353 ~ The radii and spectra of the nearest stars. ZAKHOZHAJ V.A.
2004AJ....128..463R viz 15       D               1079 147 Meeting the cool neighbors. VIII. A preliminary 20 parsec census from the NLTT catalogue. REID I.N., CRUZ K.L., ALLEN P., et al.
2008MNRAS.389..925T viz 15       D               1 1502 160 Comparative statistics and origin of triple and quadruple stars. TOKOVININ A.
2010MNRAS.403.1089P viz 15       D               1 851 46 Target selection for the SUNS and DEBRIS surveys for debris discs in the solar neighbourhood. PHILLIPS N.M., GREAVES J.S., DENT W.R.F., et al.
2011A&A...532A...6S 77             C       1 196 298 Estimation of the XUV radiation onto close planets and their evaporation. SANZ-FORCADA J., MICELA G., RIBAS I., et al.
2012ApJ...753..156K viz 15       D               2 485 288 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.
2012AJ....144...64D viz 15       D               1 241 81 The solar neighborhood. XXVIII. The multiplicity fraction of nearby stars from 5 to 70 AU and the brown dwarf desert around M dwarfs. DIETERICH S.B., HENRY T.J., GOLIMOWSKI D.A., et al.
2012A&A...546A..69M viz 15       D               2 3267 83 Dynamical masses of a selected sample of orbital binaries. MALKOV O.Yu., TAMAZIAN V.S., DOCOBO J.A., et al.
2013ApJ...766...69L 39           X         1 50 65 Computing intrinsic Lyα fluxes of F5 V to M5 V stars. LINSKY J.L., FRANCE K. and AYRES T.
2013AJ....146...99C 94       D       C       3 162 14 The solar neighborhood XXIX: the habitable real estate of our nearest stellar neighbors. CANTRELL J.R., HENRY T.J. and WHITE R.J.
2015ApJ...810..106M 40           X         1 4 5 Eccentricity evolution through accretion of protoplanets. MATSUMOTO Y., NAGASAWA M. and IDA S.
2016MNRAS.463.1592C 80           X         2 11 5 Spin-orbit evolution of the GJ 667C system: the effect of composition and other planets' perturbations. CUARTAS-RESTREPO P.A., MELITA M., ZULUAGA J.I., et al.
2017A&A...600A..22M viz 43           X         1 13 33 The AMBRE project: Iron-peak elements in the solar neighbourhood. MIKOLAITIS S., DE LAVERNY P., RECIO-BLANCO A., et al.
2017ApJ...844..103T viz 1163 56 Orbit alignment in triple stars. TOKOVININ A.
2021A&A...650A.201R viz 17       D               1 532 36 The 10 parsec sample in the Gaia era. REYLE C., JARDINE K., FOUQUE P., et al.
2023A&A...680A..64D 47           X         1 93 ~ Planetary system architectures with low-mass inner planets Direct imaging exploration of mature systems beyond 1 au. DESGRANGE C., MILLI J., CHAUVIN G., et al.

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