Results 1 to 10 of about 43,803 (189)
Chemically Peculiar Stars Among Spectroscopic Binaries – Revisited [PDF]
AbstractThis paper presents a new statistical investigation of peculiar A-type stars (Am, Ap, Hg-Mn) among spectroscopic binary (SB) stars. The relative frequency of Am (CP 1) stars is 55% in the spectral range A1 to A6 of main-sequence stars. The Ap (CP 2) stars amount to 15% in the range B9 to A2.
W. Seggewiß
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SPECTROSCOPIC METALLICITY DETERMINATIONS FOR W UMa-TYPE BINARY STARS [PDF]
This study is an attempt to determine the metallicities of WUMa-type binary stars using spectroscopy. ~4,500 spectra collected at the David Dunlap Observatory were subject to the same Broadening Function processing to determine the combined line strength in the spectral window centered on the MgI triplet (5080-5285A).
S. M. Ruciński, T. Pribulla, J. Budaj
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The Smallest Mass Ratio Young Star Spectroscopic Binaries [PDF]
Accepted for publication in the April, 2002, ApJ; 6 ...
Tsevi Mazeh+5 more
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A Survey for Spectroscopic Binaries among Very Low Mass Stars [PDF]
We report on the results of a survey for radial velocity variability in a heterogeneous sample of very low-mass stars and brown dwarfs. One distinguishing characteristic of the survey is its timespan, which allows an overlap between spectroscopic binaries and those which can be found by high angular-resolution imaging.
Gibor Basri, A. Reiners
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THREE SPECTROSCOPIC BINARY STARS. [PDF]
Roscoe F. Sanford
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Binary Star Orbits. VI. The Interferometric-spectroscopic Binary 73 Leo
Discordances in radial-velocity measurements of 73 Leonis, made more than a century ago, gave rise to the first suggestion that this fifth-magnitude star was a binary system, but it was 40 yr before an accurate investigation of the object commenced, and ...
Brian D. Mason+9 more
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A Survey for Young Spectroscopic Binary K7–M4 Stars in Ophiuchus [PDF]
30 pages, 6 figures; accepted in Astrophysical ...
L. Prato
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The CARMENES search for exoplanets around M dwarfs: Nine new double-line spectroscopic binary stars
Context. The CARMENES spectrograph is surveying ~300 M dwarf stars in search for exoplanets. Among the target stars, spectroscopic binary systems have been discovered, which can be used to measure fundamental properties of stars. Aims.
D. Baroch+29 more
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A STUDY OF SPECTROSCOPIC BINARY STARS [PDF]
W. W. Campbell
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NEW SPECTROSCOPIC BINARY STARS. [PDF]
H. M. Reese
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