Stellar Outflows Driven by Radiation Pressure
@article{Ivezi1998StellarOD,
title={Stellar Outflows Driven by Radiation Pressure},
author={Željko Ivezi{\'c} and Gillian R. Knapp and Moshe Elitzur},
journal={arXiv: Astrophysics},
year={1998}
}We present a detailed, self-consistent model of radiatively driven stellar outflows which couples the radiative transfer and hydrodynamics equations. The circumstellar envelope, which consists of gas and dust, is described as a two-component fluid to account for relative drifts. Our results agree with both molecular line observations and infrared continuum spectra, and show that steady-state outflows driven by radiation pressure on dust grains adequately describe the surroundings of the…
One Citation
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