Stellar Outflows Driven by Radiation Pressure

Simple item page
dc.creatorIvezic, Z.
dc.creatorKnapp, G. R.
dc.creatorElitzur, M.
dc.date1998-05-01
dc.date.accessioned2026-07-07T02:26:43Z
dc.date.available2026-07-07T02:26:43Z
dc.descriptionWe 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 majority of cool luminous evolved stars.
dc.description5 pages with 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9805003
dc.identifierhttp://arxiv.org/abs/astro-ph/9805003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12392
dc.subjectAstrophysics
dc.titleStellar Outflows Driven by Radiation Pressure
dc.typetext

Files

Collections

arXiv