Volume 569, September 2014
|Number of page(s)||6|
|Section||Stellar structure and evolution|
|Published online||02 October 2014|
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.
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⊙.
© ESO, 2014
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.