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A Spectrophotometer Devoted to Stellar Seismology

Published online by Cambridge University Press:  12 April 2016

Eric Fossat ,
Yves Decanini  and
Gérard Grec
Eric Fossat
Affiliation:
Observatoire de Nice, B.P.252 – 06007 NICE Cedex – France
Yves Decanini
Affiliation:
Département d'Astrophysique de l'I.M.P.S., Parc Valrose 06034 NICE Cedex - France, Equipe de Recherche Associée n° 669 du C.N.R.S.
Gérard Grec
Affiliation:
Département d'Astrophysique de l'I.M.P.S., Parc Valrose 06034 NICE Cedex - France, Equipe de Recherche Associée n° 669 du C.N.R.S.

Extract

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I wish to begin by saying a few words on an instrument which has been utilized thus far only to observe the sun, with a very small telescope of about 5cm diameter. This may appear to stand far away from the main topic of this meeting but in fact, the scientific program which is successfully being developed on the sun would be of major interest for stellar astronomy if it could be extended to at least a few bright stars. I will therefore describe also a possible extrapolation of an instrument to be used on the largest available telescopes for stellar observations.

Information

Type
Section II: Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 67: Instrumentation for Astronomy with Large Optical Telescopes , 1982 , pp. 169 - 174
Copyright
Copyright © Reidel 1982

References

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