Data for computing radiation forces on highly ionized elements

Details Data for computing radiation forces on highly ionized elements Data for computing radiation forces on highly ionized elements

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...83..379a&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 83, no. 2, May 1990, p. 379-390.

Astronomy and Astrophysics

Astrophysics

3

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

Scientific paper

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 main-sequence stars with effective temperatures of 7240 K, 10,000 K, 12,000 K, and 14,000 K. The coefficients Phi-asterisk and Psi-asterisk defined by Alecian and Artru (1990) are obtained for 21 isoelectronic sequences (from He-like through Ti-like).

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