Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-30T00:46:38.211Z Has data issue: false hasContentIssue false
  • English
  • Français

The rich p-mode pulsation spectrum of HD 60435

Published online by Cambridge University Press:  03 August 2017

J.M. Matthews ,
D.W. Kurtz  and
W.H. Wehlau
J.M. Matthews
Affiliation:
University of Western Ontario
D.W. Kurtz
Affiliation:
University of Cape Town
W.H. Wehlau
Affiliation:
University of Western Ontario

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Twelve cool Ap stars are known at present to undergo rapid light oscillations at low amplitude (ΔB < 0m.012) and with periods of minutes. These rapidly oscillating Ap (roAp) stars also exhibit amplitude modulation with timescales of days, which correspond to the magnetic/rotation periods (when those have been measured). In at least one case (HR 3831), 180° phase shifts in the dominant oscillation are seen twice per modulation cycle.

Type
Chapter 4: Asteroseismology: Results and Prospects
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 261 - 264
Copyright
Copyright © Reidel 1988 

References

Deeming, T.J. 1975. Ap. Space Sci. 36, 137.CrossRefGoogle Scholar
Dolez, N. and Gough, D.O. 1982. in Pulsations in Classical and Cataclysmic Variables, eds. Cox, and Hansen, (Boulder: JILA), 248.Google Scholar
Gabriel, M., Noels, A., Scuflaire, R. and Mathys, G. 1985. Astron. Astrophys. 143, 206.Google Scholar
Kurtz, D.W. 1982. M.N.R.A.S. 200, 807.CrossRefGoogle Scholar
Kurtz, D.W. 1984. M.N.R.A.S. 209, 841.CrossRefGoogle Scholar
Matthews, J.M. and Wehlau, W.H. 1985. P.A.S.P. 97, 841.CrossRefGoogle Scholar
Matthews, J.M., Kurtz, D.W. and Wehlau, W.H. 1986. Ap. J. 300, 348.CrossRefGoogle Scholar
Shibahashi, H. and Saio, H. 1985. Publ. Astron. Soc. Japan 37, 245.Google Scholar