Connection between nonradial pulsations and stellar winds in massive stars. V - Stellar winds and variability in hot luminous stars

Details Connection between nonradial pulsations and stellar winds in massive stars. V - Stellar winds and variability in hot luminous stars Connection between nonradial pulsations and stellar winds in massive stars. V - Stellar winds and variability in hot luminous stars

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98...41c&link_type=abstract

(Workshop on the Connection between Nonradial Pulsations and Stellar Winds in Massive Stars, Boulder, CO, Apr. 17-19, 1985) Astr

Astronomy and Astrophysics

Astronomy

2

Hot Stars, Stellar Luminosity, Stellar Mass Ejection, Stellar Spectrophotometry, Stellar Winds, Wolf-Rayet Stars, B Stars, Emission Spectra, Line Spectra, O Stars, Periodic Variations, Radial Velocity, Spaceborne Astronomy, Spectral Energy Distribution, Very Large Array (Vla)

Scientific paper

Progress made in the determination of mass-loss rates, terminal velocities, and other parameters in the winds of the OB stars and the Wolf-Rayet (W-R) objects is considered. It is thought best to base mass-loss rates on the observations of the free-free emission of electrons in the winds, taking into account, for example, a detection in the radio wavelengths on the Very Large Array. It is found that mass-loss rates in hot stars depend on luminosity to some power. All of the studies, both observational and theoretical, have ignored the issues of variability.Questions regarding variability are examined, and requirements for its observation are discussed.

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