Data for computing radiation forces on highly ionized elements
Abstract
This paper gives results of an extensive computation of coefficients useful for computing radiation forces on highly ionized elements in stellar envelopes. Tables of results are provided for four different models of mainsequence stars with effective temperatures of 7240 K, 10,000 K, 12,000 K, and 14,000 K. The coefficients Phiasterisk and Psiasterisk defined by Alecian and Artru (1990) are obtained for 21 isoelectronic sequences (from Helike through Tilike).
 Publication:

Astronomy and Astrophysics Supplement Series
 Pub Date:
 May 1990
 Bibcode:
 1990A&AS...83..379A
 Keywords:

 Ionized Gases;
 Main Sequence Stars;
 Stellar Envelopes;
 Abundance;
 Astronomical Models;
 Electron Transitions;
 Stellar Temperature;
 Astrophysics