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Description
  • We study the effect of wind inhomogeneities (clumping) on O star wind model predictions. For this purpose we artificially include clumping into our stationary NLTE wind models. As a result of the inclusion of optically thin clumps the radiative line force is increased compared to corresponding unclumped models, with a similar effect on either the mass-loss rate or the terminal velocity. When the clumps are allowed to be optically thick in continuum, on the other hand, the radiative force and consequently the mass-loss rate decreases alternatively.
  • We study the effect of wind inhomogeneities (clumping) on O star wind model predictions. For this purpose we artificially include clumping into our stationary NLTE wind models. As a result of the inclusion of optically thin clumps the radiative line force is increased compared to corresponding unclumped models, with a similar effect on either the mass-loss rate or the terminal velocity. When the clumps are allowed to be optically thick in continuum, on the other hand, the radiative force and consequently the mass-loss rate decreases alternatively. (en)
Title
  • The influence of inhomogeneities on hot star wind model predictions
  • The influence of inhomogeneities on hot star wind model predictions (en)
skos:prefLabel
  • The influence of inhomogeneities on hot star wind model predictions
  • The influence of inhomogeneities on hot star wind model predictions (en)
skos:notation
  • RIV/00216224:14310/08:00025134!RIV10-GA0-14310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/07/0031), P(GA205/08/0003), Z(AV0Z10030501)
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 372144
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/08:00025134
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars: winds; outflows stars: mass-loss; stars: early-type; hydrodynamics (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [BA43F08213E4]
http://linked.open...v/mistoKonaniAkce
  • Sanya, Čína
http://linked.open...i/riv/mistoVydani
  • Cambridge, United Kingdom
http://linked.open...i/riv/nazevZdroje
  • The Art of Modelling Stars in the 21st Century
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Krtička, Jiří
  • Kubát, Jiří
  • Muijres, Lianne
  • Puls, Joachim
  • de Koter, Alex
http://linked.open...vavai/riv/typAkce
http://linked.open...ain/vavai/riv/wos
  • 000263138600056
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
number of pages
http://purl.org/ne...btex#hasPublisher
  • Cambridge University Press
https://schema.org/isbn
  • 978-0-521-88983-4
http://localhost/t...ganizacniJednotka
  • 14310
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