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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
Abstract
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
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- Copyright © Astronomical Society of the Pacific 2002