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Interferometry of Cool Pulsating Stars

Published online by Cambridge University Press:  12 April 2016

Chris Haniff
Chris Haniff*
Affiliation:
Mullard Radio Astronomy Observatory, University of Cambridge, Cavendish Laboratory, Madingley Road, Cambridge, CB3 OHE, England

Abstract

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The drive for high-angular resolution from the ground has led to the development of optical and near infrared interferometric telescopes analogous to radio synthesis arrays. These now provide a diffraction-limited imaging capability well suited to studies of nearby cool giants and supergiants. In this review I summarise the current status of these instruments, their scientific potential for studies of cool pulsating variables (LPVs), and present some recent results that highlight the promise that such methods hold.

Type
Part 1. The Scientific Programme
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 270 - 280
Copyright
Copyright © Astronomical Society of the Pacific 1995

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