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Spectroscopic Survey of Rapidly Oscillating Ap Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
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A spectroscopic survey of roAp stars has been initiated in Vienna in order to determine their fundamental astrophysical parameters and abundances. We report here on our attempt to confirm and elaborate an atmospheric peculiarity recently discovered (Ryabchikova et al. 1999) which should allow to identify roAp stars with a single spectrum.
- Type
- Part 6. Variables Close to the Main Sequence
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
Piskunov, N.E.
1999, in ASSL Vol. 243, Proc. 2nd Int. Workshop on Solar Polarization, Bangalore, India 1998, ed. Nagendra, K. N. & Stenflo, J. O. (Dordrecht: Kluwer), 515
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Ryabchikova, T.A., Savanov, I.S., Malanushenko, V.P., & Kudryavtsev, D.A.
1999, Astronomy Reports, in pressGoogle Scholar
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