Hostname: page-component-6bf8c574d5-685pp Total loading time: 0 Render date: 2025-03-07T02:40:39.343Z Has data issue: false hasContentIssue false
  • English
  • Français

SUSI’s Potential for Cepheid Studies

Published online by Cambridge University Press:  12 April 2016

A.J. Booth ,
J. Davis  and
R.R. Shobbrook
A.J. Booth
Affiliation:
Chatterton Astronomy Department, School of Physics, University of Sydney, NSW 2006, Australia
J. Davis
Affiliation:
Chatterton Astronomy Department, School of Physics, University of Sydney, NSW 2006, Australia
R.R. Shobbrook
Affiliation:
Chatterton Astronomy Department, School of Physics, University of Sydney, NSW 2006, Australia

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.

The Sydney University Stellar Interferometer (SUSI) is the first instrument with sufficient resolving power to measure the angular sizes of a large number of stars over the full range of spectral classes. It can also resolve the orbits of spectroscopic binaries, allowing masses and distances to be determined directly. One of the major programs envisaged for the instrument is a study of pulsating stars, in particular Cepheids.

Type
Part 1. The Scientific Programme
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 281 - 282
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Albrow, M.D., & Cottrell, P.L. 1995, MNRAS, submittedGoogle Scholar
Butler, R.P. 1993, ApJ, 415, 323 Google Scholar
Davis, J., Tango, W.J, Booth, A.J., Minard, R., ten Brummelaar, T., Owens, S.M., & Shobbrook, R.R. 1995, MNRAS, in preparationGoogle Scholar
Fried, D.L. 1965, J. Opt. Soc. Am., 55, 1427 Google Scholar
Sasselov, D.D., & Karovska, M. 1994, ApJ, 432, 367 Google Scholar
Sasselov, D.D., & Lester, J.B. 1990, ApJ, 362, 333 Google Scholar