Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-26T04:39:07.712Z Has data issue: false hasContentIssue false
  • English
  • Français

Probing the interiors of roAp stars: stellar tubas that sound like piccolos

Published online by Cambridge University Press:  25 May 2016

Jaymie M. Matthews
Jaymie M. Matthews*
Affiliation:
University of British Columbia, Department of Physics & Astronomy, 2219 Main Mall, Vancouver, B.C., V6T 1Z4, Canada

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.

Chemically peculiar magnetic (Ap) stars in the Instability Strip shouldn't really pulsate (since the helium in their very stable atmospheres appears to have gravitationally settled below the He II ionisation zone). And if they did pulsate, they should have periods of a few hours like the δ Scuti variables, since the Ap stars have comparable mean densities and their atmospheric peculiarities wouldn't strongly affect the global eigenfunctions of low-degree p-modes.

Type
Part VI: Results on some selected types of stars
Information
Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 387 - 394
Copyright
Copyright © Kluwer 1997 

References

Audard, N. & Provost, J. (1993) ASPC 40, pp. 544–546.Google Scholar
Audard, N., Provost, J. & Christensen-Dalsgaard, J. (1995) A&A 297, pp. 427–440.Google Scholar
Carlberg, R. (1975) , .Google Scholar
Das, M.K., Kar, J. & Tandon, J.N. (1984) ApJ 281, pp. 292–302.CrossRefGoogle Scholar
Christensen-Dalsgaard, J. (1993) ASPC 40, pp. 483–496.Google Scholar
Dziembowski, W. & Goode, P. (1996) ApJ 458, pp. 338–346.CrossRefGoogle Scholar
Kurtz, D.W. (1990) ARA&A 28, pp. 607–655.Google Scholar
Kurtz, D.W. & Medupe, R. (1999), Bull. Astron. Soc. India, 24.Google Scholar
Kurtz, D.W., Sullivan, D.J., Martinez, P. & Tripe, P. (1994) MNRAS 270, pp. 647–686.CrossRefGoogle Scholar
Martinez, P. & Kurtz, D.W. (1995) ASPC 83, pp. 58–69.Google Scholar
Matthews, J.M. (1993) ASPC 42, pp. 303–316.Google Scholar
Matthews, J.M. & Scott, S. (1995) ASPC 83, pp. 347–348.Google Scholar
Matthews, J.M., Wehlau, W.H., Rice, J. & Walker, G.A.H. (1996) ApJ 459, pp. 278–287.CrossRefGoogle Scholar
Matthews, J.M., Wehlau, W.H. & Walker, G.A.H. (1990) ApJL 365, pp. L81–L86.CrossRefGoogle Scholar
Muthsam, H. & Stepień, K. (1992) Acta. Astron. 42, pp. 117–130.Google Scholar
Rice, J.B. & Wehlau, W.H. (1991) A&A 246, pp. 195–205.Google Scholar
Roxburgh, I. (1965) in Stellar and Solar Magnetic Fields, ed. Lüst, R., North-Holland Publishing Company, Amsterdam, pp. 103–116.Google Scholar
Shibahashi, H. & Saio, H. (1985) PASJ 37, pp. 245–255.Google Scholar
Tassoul, M. (1990) ApJ 358, pp. 313–327.CrossRefGoogle Scholar