Free Access
Issue
A&A
Volume 569, September 2014
Article Number A123
Number of page(s) 6
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201323309
Published online 02 October 2014

Online material

Appendix A: Excited modes for different spherical degrees

In this Appendix, we provide detailed information on the model with a total mass of 0.47 M and an envelope mass of 9.0 ×10-5 M, for which the pulsational characteristics were shown in Fig. 6. In Tables A.1 and A.2 the period range and the number of excited modes is given for p- and g-modes, respectively. The tables also list the effective temperature (Teff), surface gravity (log g) and Fe and Ni abundance enhancements (XFe/XFe,init and XNi/XNi,init) in the driving region as a function of time.

Table A.1

Number (No.), period range (p), and order range (n) of excited p-modes for different spherical degrees for the evolutionary track with a total mass of 0.47 M and an envelope mass of 9.0 × 10-5 M.

Table A.2

Same as Table A.1 but for excited g-modes.


© ESO, 2014

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