STELLAR ASTROPHYSICS WITH A DISPERSED FOURIER TRANSFORM SPECTROGRAPH. II. ORBITS OF DOUBLE-LINED SPECTROSCOPIC BINARIES

@article{Behr2011STELLARAW,
  title={STELLAR ASTROPHYSICS WITH A DISPERSED FOURIER TRANSFORM SPECTROGRAPH. II. ORBITS OF DOUBLE-LINED SPECTROSCOPIC BINARIES},
  author={B. Behr and A. Cenko and A. Hajian and R. McMillan and M. Murison and Jeff T. Meade and R. Hindsley},
  journal={The Astronomical Journal},
  year={2011},
  volume={142},
  pages={6}
}
We present orbital parameters for six double-lined spectroscopic binaries (ι Pegasi, ω Draconis, 12 Bootis, V1143 Cygni, β Aurigae, and Mizar A) and two double-lined triple star systems (κ Pegasi and η Virginis). The orbital fits are based upon high-precision radial velocity (RV) observations made with a dispersed Fourier Transform Spectrograph, or dFTS, a new instrument that combines interferometric and dispersive elements. For some of the double-lined binaries with known inclination angles… Expand
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References

SHOWING 1-10 OF 35 REFERENCES
The Spectroscopic and Astrometric Orbits of HR 672
PHASES Differential Astrometry and Iodine Cell Radial Velocities of the κ Pegasi Triple Star System
The double-lined spectroscopic binary IOTA Pegasi.
...
1
2
3
4
...