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Proceedings Paper

Determining the orientation of the rotation axis of a star using a spectral-line interferometer
Author(s): David J. Westpfahl; David Mozurkewich; Charles Dudley
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Paper Abstract

An optical interferometer with long baselines and high spectral resolution could be used to determine the rotation rate of a star and the orientation of its rotation axis. Orientation is information that has previously been determined only statistically for single stars. Knowing the orientation would allow solution of currently intractable problems in star formation and stellar evolution.

Paper Details

Date Published: 21 February 2003
PDF: 3 pages
Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); doi: 10.1117/12.459936
Show Author Affiliations
David J. Westpfahl, Magdalena Ridge Observatory/New Mexico Institute of Mining and Technology (United States)
David Mozurkewich, Naval Research Lab. (United States)
Charles Dudley, Naval Research Lab. (United States)


Published in SPIE Proceedings Vol. 4838:
Interferometry for Optical Astronomy II
Wesley A. Traub, Editor(s)

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