Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-29T07:18:33.559Z Has data issue: false hasContentIssue false
  • English
  • Français

Rotational Velocities of B, A, and Early-F Stars

Published online by Cambridge University Press:  26 May 2016

Francis C. Fekel ,
Phillip B. Warner  and
Anthony B. Kaye
Francis C. Fekel
Affiliation:
Tennessee State University, Center of Excellence in Information Systems, Nashville, Tennessee 37203, USA
Phillip B. Warner
Affiliation:
Department of Physics and Astronomy, Brigham Young University, Provo, Utah 84602 USA
Anthony B. Kaye
Affiliation:
Applied Physics Division, Los Alamos National Lab., X-5, MS F-663, Los Alamos, New Mexico 87545 USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Projected rotational velocities for 67 B, A, and early-F stars have been determined. Some of these stars are early-type, radial-velocity standard candidates. The spectra of seven stars show metallic lines with composite profiles that consist of a narrow component near the center of a broad component, suggesting that they may be shell stars or binaries.

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 53 - 54
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Fekel, F. C. 1997, PASP 109, 514 Google Scholar