z-logo
open-access-imgOpen Access
First Results from the CHARA Array. I. An Interferometric and Spectroscopic Study of the Fast Rotator α Leonis (Regulus)
Author(s) -
Harold A. McAlister,
Theo A. ten Brummelaar,
Douglas R. Gies,
W. Huang,
W. G. Bagnuolo,
M. A. Shure,
J. Sturmann,
L. Sturmann,
N. H. Turner,
Stuart F. Taylor,
David H. Berger,
Ellyn K. Baines,
Erika D. Grundstrom,
Chad Ogden,
Stephen T. Ridgway,
Gerald van Belle
Publication year - 2005
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/430730
Subject(s) - interferometry , physics , position angle , astrophysics , polar , astronomy , optics , galaxy
We report on K-band interferometric observations of the bright, rapidlyrotating star Regulus (type B7 V) made with the CHARA Array on Mount Wilson,California. Through a combination of interferometric and spectroscopicmeasurements, we have determined for Regulus the equatorial and polar diametersand temperatures, the rotational velocity and period, the inclination andposition angle of the spin axis, and the gravity darkening coefficient. Thesefirst results from the CHARA Array provide the first interferometricmeasurement of gravity darkening in a rapidly rotating star and represent thefirst detection of gravity darkening in a star that is not a member of aneclipsing binary system.Comment: Accepted for publication in The Astrophysical Journal, 44 pages w/ 14 figure

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom