SB9: The Ninth Catalogue of Spectroscopic Binary Orbits

Abstract

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 2,386 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.

Accepte for publication in A&A, 6 pages, 6 figures

Cited by in corpus (393)

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• Spectroscopic orbit determination of the long-periodic binary system $\theta$ Cep
• Variable binaries and variables in binaries in the Binary Star Database BDB
• Comprehensive study of five candidate delta Scuti-type pulsators in detached eclipsing binaries
• Analysis of Gaia radial-velocity standards: stability and new substellar companion candidates
• The Gaia-ESO Survey: new spectroscopic binaries in the Milky Way
• Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
• Filling the gap: the missing eclipses of $\gamma$ Persei from 2005 and from 2006
• SPORES-HWO. II. Companion Mass Limits and Updated Planet Properties for 120 Future Exoplanet Imaging Targets from 35 yr of Precise Doppler Monitoring
• Separated Fringe Packet Observations with the CHARA Array III. The Very High Eccentricity Binary HR 7345
• Binary Star Database (BDB): New Developments and Applications
• Precise Physical Parameters, Habitability, and Orbital Stability of Sun-like SB2 Systems: HD 130669, HD 184467, HD 191854, and HD 214222
• Kinematics of nearby OB3 stars with interstellar CaII line distances
• Analysis of the multiple system with CP component phi Draconis
• The Solar Neighborhood. LV. M Dwarf Twin Binaries -- One in Five Twin Sibling Pairs Are Mismatched in Activity and/or Rotation
• Red giant asteroseismic binaries in the Kepler field
• Double-lined spectroscopic binaries in the APOGEE DR16 and DR17 data
• Two unseen massive white dwarf candidates in close binaries
• ExoDNN: Boosting exoplanet detection with artificial intelligence. Application to Gaia Data Release 3
• The peculiar nebula Simeis 57: II. Distance, nature and excitation
• Activity cycles in RS CVn type stars
• Double-lined spectroscopic binaries in M11
• Identification of additional young nearby runaway stars based on Gaia data release 2 observations and the lithium test
• Syntriod: A Robust Initial Parameter Estimator for Radial Velocity Curve Solutions Beyond Conventional Sampling Limits
• The reason for the occurrence of W-type contact binaries
• Photometric and Spectroscopic Analysis of Five Am Stars
• Study of Massive OBA Stars with X-ray Emission
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• Bayesian inference in single-line spectroscopic binaries with a visual orbit
• Looking for Signs of Unresolved Binarity in the Continuum of LAMOST Stellar Spectra
• CoronaGraph Instrument Reference stars for Exoplanets (CorGI-REx) I. Preliminary Vetting and Implications for the Roman Coronagraph and Habitable Worlds Observatory
• An Adaptive Optics Census of Companions to Northern Stars Within 25 pc with Robo-AO
• Identification of false positive double-lined spectroscopic binaries in LAMOST-MRS data due to moonlight contamination
• Kinematics of the Central Stars Powering Bowshock Nebulae and the Large Multiplicity Fraction of Runaway OB Stars
• A 2+1+1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known