DOUBLE-LINED SPECTROSCOPIC BINARY STARS IN THE RAVE SURVEY

@article{Matijevi2010DOUBLELINEDSB,
  title={DOUBLE-LINED SPECTROSCOPIC BINARY STARS IN THE RAVE SURVEY},
  author={Gal Matijevi{\vc} and Toma{\vz} Zwitter and U. Munari and Olivier Bienaym{\'e} and James Binney and J. Bland-Hawthorn and Corrado Boeche and R. Campbell and Kenneth C. Freeman and Brad K. Gibson and Gerry F. Gilmore and Eva K. Grebel and Amina Helmi and Julio F. Navarro and Quentin A. Parker and George Mitchell Seabroke and Arnaud Siebert and Alessandro Siviero and Matthias Steinmetz and Fred G. Watson and M. E. K. Williams and R. F. G. Wyse},
  journal={The Astronomical Journal},
  year={2010},
  volume={140},
  pages={184-195}
}
We devise a new method for the detection of double-lined binary stars in a sample of the Radial Velocity Experiment (RAVE) survey spectra. The method is both tested against extensive simulations based on synthetic spectra and compared to direct visual inspection of all RAVE spectra. It is based on the properties and shape of the cross-correlation function, and is able to recover ~80% of all binaries with an orbital period of order 1 day. Systems with periods up to 1 yr are still within the… Expand

Figures and Tables from this paper

SINGLE-LINED SPECTROSCOPIC BINARY STAR CANDIDATES IN THE RAVE SURVEY
Repeated spectroscopic observations of stars in the RAdial Velocity Experiment (RAVE) database are used to identify and examine single-lined binary (SB1) candidates. The RAVE latest internal databaseExpand
Double-lined Spectroscopic Binaries in the APOGEE DR16 and DR17 Data
APOGEE spectra offer ≲1 km s−1 precision in the measurement of stellar radial velocities. This holds even when multiple stars are captured in the same spectrum, as happens most commonly withExpand
Single-lined Spectroscopic Binary Star Candidates from a Combination of the RAVE and Gaia DR2 Surveys
The combination of the final version of the RAVE spectroscopic survey data release 6 with radial velocities and astrometry from Gaia DR2 allows us to identify and create a catalog of single linedExpand
CHROMOSPHERICALLY ACTIVE STARS IN THE RADIAL VELOCITY EXPERIMENT (RAVE) SURVEY. I. THE CATALOG
RAVE, the unbiased magnitude limited survey of southern sky stars, contained 456,676 medium-resolution spectra at the time of our analysis. Spectra cover the Ca II infrared triplet (IRT) range, whichExpand
The Gaia-ESO Survey: double, triple and quadruple-line spectroscopic binary candidates
The Gaia-ESO Survey (GES) is a large spectroscopic survey that provides a unique opportunity to study the distribution of spectroscopic multiple systems among different populations of the Galaxy. WeExpand
Distance determination for RAVE stars using stellar models . II. Most likely values assuming a standard stellar evolution scenario
The RAdial Velocity Experiment (RAVE) is a spectroscopic survey of the Milky Way which already collected over 400000 spectra of ∼330000 different stars. We use the subsample of spectra withExpand
Very metal-poor stars observed by the RAVE survey
Metal-poor stars trace the earliest phases in the chemical enrichment of the Universe. They give clues about the early assembly of the Galaxy as well as on the nature of the first stellarExpand
The GALAH survey: unresolved triple Sun-like stars discovered by the Gaia mission
The latest Gaia data release enables us to accurately identify stars that are more luminous than would be expected on the basis of their spectral type and distance. During an investigation of theExpand
Refined Metallicity Indices for M Dwarfs Using the SLoWPoKES Catalog of Wide, Low-mass Binaries
We report the results from spectroscopic observations of 113 ultra-wide, low-mass binary systems, largely composed of M0-M3 dwarfs, from the SLoWPoKES catalog of common proper motion pairs identifiedExpand
Observational Properties of the Metal-poor Thick Disk of the Milky Way and Insights into its Origins
We have undertaken the study of the elemental abundances and kinematic properties of a metalpoor sample of candidate thick-disk stars selected from the RAVE spectroscopic survey of bright stars toExpand
...
1
2
3
...

References

SHOWING 1-10 OF 27 REFERENCES
SINGLE-LINED SPECTROSCOPIC BINARY STAR CANDIDATES IN THE RAVE SURVEY
Repeated spectroscopic observations of stars in the RAdial Velocity Experiment (RAVE) database are used to identify and examine single-lined binary (SB1) candidates. The RAVE latest internal databaseExpand
Diffuse interstellar bands in RAVE survey spectra
We have used spectra of hot stars from the RAVE Survey in order to investigate the visibility and properties of five diffuse interstellar bands previously reported in the literature. The RAVEExpand
Asiago eclipsing binaries program II. V505 Persei
The orbit and fundamental physical parameters of the double-lined eclipsing binary V505 Per are derived by means of Echelle highresolution and high S /N spectroscopy, and B, V photometry. InExpand
RAVE spectroscopy of luminous blue variables in the Large Magellanic Cloud
Context. The RAVE spectroscopic survey for galactic structure and evolution obtains 8400-8800 A spectra at 7500 resolving power at the UK Schmidt Telescope using the 6dF multi-fiber positioner. Mor eExpand
The radial velocity experiment (RAVE): First data release
TLDR
The first data release of the Radial Velocity Experiment (RAVE) is presented and it is demonstrated that the radial velocities derived for the first data set do not show any systematic trend with color or signal-to-noise ratio. Expand
Distance determination for RAVE stars using stellar models
Aims. We develop a method for deriving distances from spectroscopic data and obtaining full 6D phase-space coordinates for the RAVE survey’s second data release. Methods. We used stellar modelsExpand
A SPECTROSCOPIC SURVEY AND ANALYSIS OF BRIGHT, HYDROGEN-RICH WHITE DWARFS*
We have conducted a spectroscopic survey of over 1300 bright (V ≤ 17.5), hydrogen-rich white dwarfs based largely on the last published version of the McCook & Sion catalog. The complete results fromExpand
A catalogue of chromospherically active binary stars (third edition)
The catalogue of chromospherically active binaries (CABs) has been revised and updated. With 203 new identifications, the number of CAB stars is increased to 409. The catalogue is available inExpand
The RAVE survey: constraining the local Galactic escape speed
TLDR
New constraints on the local escape speed of the Galaxy are reported, finding that the escape velocity lies within the range 498 <v(esc) <608 km s (-1) (90 per cent confidence), with a median likelihood of 544 km s(-1). Expand
The distance to the Pleiades from orbital solution of the double-lined eclipsing binary HD 23642
Combining precise B,V photoelectric photometry and radial velocities, we have been able to derive a firm orbital solution and accurate physical parameters for the newly discovered eclipsing binary HDExpand
...
1
2
3
...