A Survey of Proper-Motion Stars. XVI. Orbital Solutions for 171 Single-lined Spectroscopic Binaries

By D. Latham, R. Stefanik, G. Torres, R. Davis, T. Mazeh, B. Carney, J. B. Laird, J. Morse. 2002

280 citations recorded by the source corpus.

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In Astronomy and Astrophysics

Citations in the corpus

Abundances In Very Metal-Poor Dwarf Stars (2004, background): “Latham et al. (2002) and Carney et al. (2003) find no difference in the binary frequency they establish for moderately metal poor halo populations compared to that of nearby more metal-rich populations; the formal frequency of spectroscopic binaries and multiple systems per target is 17.0±1.0%.”
The Close Binary Fraction of Solar-type Stars Is Strongly Anticorrelated with Metallicity (2018, methodology): “In particular, Latham et al. (2002) and Carney et al. (2005) investigated a large sample of 1464 FGK stars with high proper motion in the disk and halo.”
Observational Evidence for Tidal Interaction in Close Binary Systems (2007, background): “…with G-type primaries found in the solar neighbourhood (Duquennoy & Mayor 1991), in the open clusters M67 (Latham et al. 1992a,b), NGC 188 (Mathieu et al. 2004) and recently M35 (Meibom & Mathieu 2005, hereafter MM05), in PMS (Melo et al. 2001) and in the halo and field stars (Latham et al. 2002).”
ROTATIONAL AND RADIAL VELOCITIES FOR A SAMPLE OF 761 HIPPARCOS GIANTS AND THE ROLE OF BINARITY (2007, methodology): “Our techniques for identifying spectroscopic binaries were similar to those described in Latham et al. (2002) and will not be repeated in detail here.”
A Robust Measure of Tidal Circularization in Coeval Binary Populations: The Solar-Type Spectroscopic Binary Population in the Open Cluster M35 (2004, background): “From a large sample of 171 high propermotion spectroscopic binaries, Latham et al. (2002) find no obvious differences between the binary characteristics in the halo and in the disk populations.”
SPECKLE INTERFEROMETRY AT SOAR IN 2010 AND 2011: MEASURES, ORBITS, AND RECTILINEAR FITS (2012, methodology): “We combined interferometric measures with the spectroscopic data of Latham et al. (2002) which are truly complementary.”
The Rise of the s-Process in the Galaxy (2004, background): “This star does not appear to be unusual in any other respect, and Latham et al. (2002) does not identify this star as a binary.”
FROM BINARIES TO MULTIPLES. I. DATA ON F AND G DWARFS WITHIN 67 pc OF THE SUN (2014, background): “Preliminary orbital solutions for many bina- ries were obtained at Center for Astrophysics (CfA) by D. W. Latham (2012, private communication), extending the survey by Latham et al. (2002).”
OBSERVATIONS OF HIERARCHICAL SOLAR-TYPE MULTIPLE STAR SYSTEMS (2015, background): “The inner spectroscopic binary has P = 25.4 d (Latham et al. 2002), the Robo-AO companion at 5′′ is seen at a constant position despite PM(A)= 0.”
The Binary Frequency Among Carbon-enhanced, s-Process-rich, Metal-poor Stars (2004, unknown): “Latham et al. (2002) monitored HD 140283 for 3114 days with 19 observations, reported a mean radial velocity of −171.12 ± 0.29 km s−1 for this object.”
OXYGEN ABUNDANCES IN NEARBY FGK STARS AND THE GALACTIC CHEMICAL EVOLUTION OF THE LOCAL DISK AND HALO (2013, methodology): “For the other stars, we used the average of values from the following sources: Barbier-Brossat et al. (1994), Duflot et al. (1995), the Geneva-Copenhagen Survey (Nordström et al. 2004), Ramı́rez et al. (2009), Jenkins et al. (2011), Latham et al. (2002), and our own measurements.”
Stellar Multiplicity (2013, background): “SBs among Population II stars appear to be equally frequent and to share very similar properties with their higher-metallicity counterparts (Goldberg et al. 2002, Latham et al. 2002).”
HE 1327–2326, an Unevolved Star with [Fe/H] < –5.0. I. A Comprehensive Abundance Analysis (2005, methodology): “This has been measured by Latham et al. (2002) for 33 epochs covering 13 yr, and shows no clear variation.”
The RAVE Survey: Constraining the Local Galactic Escape Speed (2006, background): “These values are typical of single-lined spectroscopic binaries in Latham et al. (2002), for which 68 per cent have semi-amplitudes within the range 3–15 km s−1.”
IMPROVED SPECTROSCOPIC PARAMETERS FOR TRANSITING PLANET HOSTS (2012, background): “…Kurucz model atmospheres (Castelli & Kurucz 2003, 2004), and determines the temperature, surface gravity, metallicity, and projected rotational velocity by seeking the maximum of the cross-correlation coefficient as a function of those parameters (see also Torres et al. 2002; Latham et al. 2002).”
Tertiary Companions to Close Spectroscopic Binaries (2006, methodology): “The sample was complemented by new SBs from recent surveys of nearby stars (Latham et al. 2002; Goldberg et al. 2002; Halbwachs et al. 2003; and other).”
Elemental abundance survey of the Galactic thick disc (2005, methodology): “In the final computation of the U, V and W for the 176 stars, we made extensive use of three new sources of radial velocities: Latham et al. (2002), Nidever et al. (2002) and Nordström et al. (2004).”