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High Resolution Spectrograph Needs for Stellar Seismology

Published online by Cambridge University Press:  19 July 2016

S⊘ren Frandsen
S⊘ren Frandsen*
Affiliation:
Astronomisk Institut, Aarhus Universitet, DK-8000 Aarhus C, Denmark

Extract

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There are two ways to become a famous observing astronomer: 1) by discovering something new and exciting, 2) by detecting a phenomena, which has been predicted, but not observed before.

Type
I. Spectrographs, Detectors, Fourier Transform Spectroscopy, and Radial Velocities
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 27 - 30
Copyright
Copyright © Kluwer 1988 

References

Christensen-Dalsgaard, J., 1987a, Proc. of IAU Symposium 123: Advances in Helio- and Asteroseismology, (Eds. Christensen-Dalsgaard, J. and Frandsen, S.), Reidel, Dordrecht, to be published Google Scholar
Däppen, W., 1988, These Proceedings.Google Scholar
Frandsen, S., 1984, Proc. of the 25th Liege Int. Astroph. Coll., 303 Google Scholar
Frandsen, S., 1987, Astron. Astrophys., 181, 289 Google Scholar
Harvey, J.W., 1987, Proc. of IAU Symposium 123: Advances in Helio- and Asteroseismology, (Eds. Christensen-Dalsgaard, J. and Frandsen, S.), Reidel, Dordrecht, to be published Google Scholar
Stebbins, R., and Goode, P.R. 1987, Solar Phys., to be published Google Scholar