Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-06T01:19:03.887Z Has data issue: false hasContentIssue false

Spectroscopic Nonadiabatic Observables as a New Tool for Mode Identification in β Cep Stars

Published online by Cambridge University Press:  12 April 2016

J. Daszyńska
Affiliation:
Astronomical Institute of the Wrocław University, Poland
H. Cugier
Affiliation:
Astronomical Institute of the Wrocław University, Poland

Abstract

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.

We present a new method of mode identification based on the line profile variations. We calculate time series of Si III 455.26 nm for models of β Cep stars with a mass of 10 M. The Spectroscopic observables are amplitude ratio and phase difference for various oscillation parameters derived from the line profile changes. Based on the computed values we plot diagrams to search for the best discriminators of modes.

In most Spectroscopic diagrams the unstable modes are grouped in well-defined regions with different m-values, and a few of them give also separation with respect to l-values. Moreover, on the basis of almost all of the diagrams we can distinguish the prograde modes from the retrograde ones, and the zonal modes from those with m ≠ 0.

In this paper we discuss also the influence of the inclination angle, the amplitude of the radius variation and the equatorial velocity on the diagnostic values of the Spectroscopic diagrams.

Type
Part 2.2. B-Type Stars
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Aerts, C., De Pauw, M., & Waelkens, C. 1992, A&A, 266, 294 Google Scholar
Balona, L.A. 1986a, MNRAS, 219, 111 CrossRefGoogle Scholar
Balona, L.A. 1986b, MNRAS, 220, 647 Google Scholar
Cugier, H. & Daszyńska, J. 2001, A&A, 377, 113 Google Scholar
Cugier, H., Dziembowski, W.A., & Pamyatnykh, A.A. 1994, A&A, 266, 294 Google Scholar
Daszyńska, J. & Cugier, H. 2001, Odessa Astron. Publ., in pressGoogle Scholar
Dziembowski, W.A. & Pamyatnykh, A.A. 1993, MNRAS, 265, 588 Google Scholar
Kurucz, R.L. 1996, CD-ROM No.19Google Scholar
Ledoux, P. 1951, ApJ, 114, 373 Google Scholar
Watson, R.D. 1988, Ap&SS, 140, 255,Google Scholar