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

Published online by Cambridge University Press:  12 April 2016

Steven D. Kawaler
Steven D. Kawaler*
Affiliation:
Iowa State University, Department of Physics and Astronomy, Ames, IAUSA50011

Abstract

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The interplay between theory and observation has been particularly close in asteroseismology, ranging from white dwarfs through roAp stars. This trend should continue as the field expands to include new classes such as solar-type stars. This synergistic relationship relies on communication between theorists and observers, but also on healthy skepticism in both directions. Here, I outline a (somewhat personal) view of the theoretical side - what kinds of observations are most helpful for optimizing utility of theoretical research efforts ? Where might theory be of closer guidance as observing programs are planned ?

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. 593 - 597
Copyright
Copyright © Astronomical Society of the Pacific 2002

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