Future status of sites in asteroseismology

Details Future status of sites in asteroseismology Future status of sites in asteroseismology

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.538..381p&link_type=abstract

In: Second Eddington Workshop: Stellar structure and habitable planet finding, 9 - 11 April 2003, Palermo, Italy. Edited by F. F

Mathematics

Logic

Stars: Lambda Bootis, Stars: Beta Cephei, Stars: White Dwarfs, Stars: Gamma Doradus

Scientific paper

A possible contribution by a team at Konkoly Observatory of the Hungarian Academy of Sciences to the ground-based support of the Eddington mission is presented for different types of asteroseismologically interesting targets, which I have obtained in the last few years. Although our observational practice covers practically the whole HR diagram (RR Lyrae, Cepheid, δ Scuti, λ Bootis, γ Doradus, SPB, β Cephei stars and white dwarfs), the examples presented here concentrate mostly on my latest work. A photoelectric photometer on a smaller telescope or a CCD/photometer on a larger telescope were used depending on the target's brightness. The different aspects of ground-based support during the preparatory work and during the mission are discussed.

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