HD 116495B , the SIMBAD biblio

HD 116495B , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.17CEST01:23:44


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Title First 3 Authors
1983ApJS...53..643J 1981 18 Predicted infrared brightness of stars within 25 parsecs of the Sun. JOHNSON H.M. and WRIGHT C.D.
1986ApJ...303..470J 83 16 An unbiased X-ray sampling of stars within 25 parsecs of the sun. JOHNSON H.M.
1993A&AS..100..343P 587 39 The importance of surface inhomogeneities for K and M dwarf chromospheric fluxes. PANAGI P.M. and MATHIOUDAKIS M.
1994RMxAA..28...43P 543 88 Statistical studies of visual double and multiple stars. II. A catalogue of nearby wide binary and multiple systems. POVEDA A., HERRERA M.A., ALLEN C., et al.
1995AJ....110.1838R viz 1848 572 The Palomar/MSU nearby-star spectroscopic survey. I. The northern M dwarfs-band strengths and kinematics. REID I.N., HAWLEY S.L. and GIZIS J.E.
1996AJ....112.2799H viz 2161 422 The Palomar/MSU nearby star spectroscopic survey. II. The southern M dwarfs and investigations of magnetic activity. HAWLEY S.L., GIZIS J.E. and REID I.N.
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.
2003A&A...397..159H 495 226 Multiplicity among solar-type stars. III. Statistical properties of the F7-K binaries with periods up to 10 years. HALBWACHS J.L., MAYOR M., UDRY S., et al.
2011AJ....142...46M viz 15       D               1 2941 4 Speckle interferometry at the U.S. Naval observatory. XVII. MASON B.D., HARTKOPF W.I. and WYCOFF G.L.
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.
2021A&A...649A...6G viz 17       D               1 89188 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2021AJ....162..260M viz 17       D               1 736 ~ Astrometric mass ratios of 248 long-period binary stars resolved in Hipparcos and Gaia EDR3. MAKAROV V.V. and FABRICIUS C.

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