Paper
21 February 2003 Spectroscopic binary stars and the CHARA array
Author Affiliations +
Abstract
Georgia State University's Center for High Angular Resolution Astronomy (CHARA) operates a multi-telescope, long-baseline, optical/infrared interferometric array on Mt. Wilson, California. Since its inception, one of the primary scientific goals for the CHARA Array has been the resolution of spectroscopic binary stars, which offer tremendous potential for the determination of fundamental parameters for stars (masses, luminosities, radii and effective temperatures). A new bibliographic catalog of spectroscopic binary orbits, including a calculated estimate of the anticipated angular separation of the components, has been produced as an input catalog in planning observations with the Array. We briefly describe that catalog, which will be made available to the community on the Internet, prior to discussing observations obtained with our 330-m baseline during the fall of 2001 of the double-lined spectroscopic systems β Aur and β Tri. We also describe the initial results of an inspection of the extrasolar planetary system υ And.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Harold A. McAlister, Theo Armand ten Brummelaar, William G. Bagnuolo Jr., David H. Berger, Thomas Fallon, A. Jerkstrand, Chad E. Ogden, Stephen T. Ridgway, J. Seymour, Judit Sturmann, Laszlo Sturmann, Stuart Taylor, and Nils Henning Turner "Spectroscopic binary stars and the CHARA array", Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); https://doi.org/10.1117/12.459117
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Stars

Spectroscopy

Visibility

Calibration

Interferometry

Chemical elements

Binary data

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