S B 9 : The ninth catalogue of spectroscopic binary orbits

By Dimitri Pourbaix, A. Tokovinin, A. H. Batten, F. Fekel, W. Hartkopf, H. Levato, N. Morrell, Guillermo Torres, S. Udry. 2004

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The Ninth Catalogue of Spectroscopic Binary Orbits (http://sb9.astro.ulb.ac.be) continues the series of compilations of spectroscopic orbits carried out over the past 35 years by Batten and collaborators. As of 2004 May 1st, the new Catalogue holds orbits for 2386 systems. Some essential differences between this catalogue and its predecessors are outlined and three straightforward applications are presented: (1) completeness assessment: period distribution of SB1s and SB2s; (2) shortest periods across the H-R diagram; (3) period-eccentricity relation.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/d1f0e06e62e44af35c22549ff72142d55b592a8b

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Citations in the corpus

RETIRED A STARS AND THEIR COMPANIONS. III. COMPARING THE MASS–PERIOD DISTRIBUTIONS OF PLANETS AROUND A-TYPE STARS AND SUN-LIKE STARS (2009, background): “…binaries and include HD 8375 (discussed in §3.1), HD 65938 (Pourbaix et al. 2004; Massarotti et al. 2008), HD 179799 (Setiawan et al. 2003b; Setiawan et al. 2004; Massarotti et al. 2008), and HD 210211 (spectroscopic triple system; Horch et al. 2002; Pourbaix et al. 2004; Massarotti et al. 2008).”
The Volume-limited A-Star (VAST) survey – I. Companions and the unexpected X-ray detection of B6–A7 stars (2011, background): “Spectroscopic binaries – unresolved with these observations – constitute a significant fraction of both samples (∼15 per cent; Pourbaix et al. 2004).”
Debris Disks in Main-Sequence Binary Systems (2006, background): “The SB9 catalog (Pourbaix et al. 2004) lists two periods for HD 29140, 1350 and 3.6 days (corresponding to orbital distances 0.04 and 3 AU), likely indicating that this system is triple.”
A STELLAR ROTATION CENSUS OF B STARS: FROM ZAMS TO TAMS (2010, methodology): “To check the detection efficiency of SBs using our 13 km s−1 criterion, we searched The Ninth Catalogue of Spectroscopic Binary Orbits6 (SB9; Pourbaix et al. 2004) for known SBs among our field B star sample.”
Rotational velocities of A-type stars - IV. Evolution of rotational velocities (2012, methodology): “The Ninth Catalog of Spectroscopic Binary Orbits (Pourbaix et al. 2004) was used to complete the identification.”
BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young Associations with 150 pc (2018, unknown): “…& Webb 2000; (42) Grenier et al. 1999; (43) Pecaut & Mamajek 2013; (44) Elliott et al. 2014; (45) Webb et al. 1999; (46) Ducourant et al. 2014; (47) Pourbaix et al. 2004; (48) Kraus & Hillenbrand 2007; (49) Luhman & Steeghs 2004; (50) Shvonski et al. 2016; (51) Pecaut, priv. comm.; (52)…”
The Occurrence and Architecture of Exoplanetary Systems (2014, background): “3 shows the eccentricity-period distribution of the same number of eclipsing binary stars, drawn randomly from the heterogeneous SB9 catalog (Pourbaix et al. 2004).”
Wide double stars - I. The spectroscopic binaries: Double stars with wide separations in the AGK3 - I. The components that are themselves spectroscopic binaries (2011, background): “These additional measurements were found in the SB9 online catalogue (Pourbaix et al. 2004); they are not reproduced here, but the references are given in the notes in Section 4.4.”
Limiting eccentricity of subparsec massive black hole binaries surrounded by self-gravitating gas discs (2011, result): “Thus, our results are likely relevant for the interpretation of the observed distribution of binary star eccentricities (e.g. Pourbaix et al. 2004).”
The M-dwarfs in Multiples (MinMs) survey – I. Stellar multiplicity among low-mass stars within 15 pc (2015, unknown): “…not fully sensitive to the bottom of the main sequence, but a lower limit on the total CSF can be estimated by combining the bound companions resolved within this study with those reported within the WDS catalogue and the Ninth catalogue of Spectroscopic Binary Orbits (SB9; Pourbaix et al. 2004).”
Tertiary Companions to Close Spectroscopic Binaries (2006, methodology): “For each SB, we determined the relevant parameters σ and ∆T either from the data given in SB9 (Pourbaix et al. 2004) or from the original publications.”
THE GALACTIC O-STAR SPECTROSCOPIC SURVEY (GOSSS). II. BRIGHT SOUTHERN STARS (2013, methodology): “Finally, when no alternative source was available, we resorted to the older compilations of Mason et al. (1998) and Pourbaix et al. (2004) to include additional information.”
How Dry is the Brown Dwarf Desert? Quantifying the Relative Number of Planets, Brown Dwarfs, and Stellar Companions around Nearby Sun-like Stars (2004, methodology): “For the stellar companion data, the single-lined (SB1) and double-lined (SB2) spectroscopic binary orbits are primarily from the Ninth Catalogue of Spectroscopic Binary Orbits (Pourbaix et al. 2004) with additional interferometric, astrometric or visual solutions from the 6th Catalog of Orbits of Vi”
Unique sextuple system: 65 Ursae Majoris (2012, background): “This is the case for 65 UMa, a system whose the close components form an eclipsing binary, and additional components found to be gravitationally bounded to this pair (Pourbaix et al., 2004).”
The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc (2019, background): “Most of the AFGK systems observed by Hipparcos that have flags in the DMSA have been further examined or re-analyzed by Pourbaix et al. (2003, 2004), Platais et al. (2003), Jancart et al. (2005), Frankowski et al. (2007), Horch et al. (2002, 2011a,b, 2015a, 2017); however, few of the M dwarf…”
LOW-MASS TERTIARY COMPANIONS TO SPECTROSCOPIC BINARIES. I. COMMON PROPER MOTION SURVEY FOR WIDE COMPANIONS USING 2MASS (2009, methodology): “Pourbaix et al. (2004) indicates that this bias begins around K spectral types.”
The VAST Survey - III. The multiplicity of A-type stars within 75 pc (2013, background): “…binaries recorded within the WashingtonDouble Star Catalog (WDS; Mason et al. 2001), the Ninth Catalogue of Spectroscopic Binary Orbits (SB9; Pourbaix et al. 2004) and eclipsing binaries within the General Catalogue of Variable Stars (GCVS; Samus et al. 2009), which are all listed in…”
Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars (2016, methodology): “We remove the five spectroscopic binaries (HIP 5348, 13165, 16611, 76267, 100221) contained in the SB9 catalog (Pourbaix et al. 2004) with known orbital periods P < 20 days.”