Radiation-driven winds of hot stars. VI - Analytical solutions for wind models including the finite cone angle effect

Details Radiation-driven winds of hot stars. VI - Analytical solutions for wind models including the finite cone angle effect Radiation-driven winds of hot stars. VI - Analytical solutions for wind models including the finite cone angle effect

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...219..205k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 219, no. 1-2, July 1989, p. 205-218.

Astronomy and Astrophysics

Astrophysics

295

Hot Stars, Stellar Radiation, Stellar Winds, Equations Of Motion, O Stars, Photosphere, Planetary Nebulae, Stellar Mass Ejection

Scientific paper

Analytical solutions for radiation-driven winds of hot stars including the important finite cone angle effect (see Pauldrach et al., 1986; Friend and Abbott, 1986) are derived which approximate the detailed numerical solutions of the exact wind equation of motion very well. They allow a detailed discussion of the finite cone angle effect and provide for given line force parameters k, alpha, delta definite formulas for mass-loss rate M and terminal velocity v-alpha as function of stellar parameters.

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