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Requirements for Future Photometric and Spectroscopic Observations for Asteroseismology: One Observer’s Perspective

Published online by Cambridge University Press:  12 April 2016

L.A. Balona
L.A. Balona*
Affiliation:
South African Astronomical Observatory, P.O. Box 9, Observatory 7935, Cape Town, South Africa

Abstract

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We discuss prospects for asteroseismology in stars for which the frequencies of pulsation lie outside the asymptotic regime. The problem of mode identification in this case is the major obstacle. Mode identification techniques from photometric and Spectroscopic observations are discussed.

Type
Part 6. Asteroseismology from Space and from the Ground
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 589 - 592
Copyright
Copyright © Astronomical Society of the Pacific 2002

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