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Description
  • We calculate multicomponent line-driven wind models of stars at extremely low metallicity suitable for massive first generation stars. For most of the models we find that the multicomponent wind nature is not important for either wind dynamics or for wind temperature stratification. However, for stars with the lowest metallicities we find that multicomponent effects influence the wind structure. These effects range from pure heating to possible fallback of the nonabsorbing wind component. We present a simple formula for the calculation of metallicity for which the multicomponent effects become important. We show that the importance of the multicomponent nature of winds of low metallicity stars is characterised not only by the low density of driving ions, but also by lower mass-loss rate.
  • We calculate multicomponent line-driven wind models of stars at extremely low metallicity suitable for massive first generation stars. For most of the models we find that the multicomponent wind nature is not important for either wind dynamics or for wind temperature stratification. However, for stars with the lowest metallicities we find that multicomponent effects influence the wind structure. These effects range from pure heating to possible fallback of the nonabsorbing wind component. We present a simple formula for the calculation of metallicity for which the multicomponent effects become important. We show that the importance of the multicomponent nature of winds of low metallicity stars is characterised not only by the low density of driving ions, but also by lower mass-loss rate. (en)
  • We calculate multicomponent line-driven wind models of stars at extremely low metallicity suitable for massive first generation stars. For most of the models we find that the multicomponent wind nature is not important for either wind dynamics or for wind temperature stratification. However, for stars with the lowest metallicities we find that multicomponent effects influence the wind structure. These effects range from pure heating to possible fallback of the nonabsorbing wind component. We present a simple formula for the calculation of metallicity for which the multicomponent effects become important. We show that the importance of the multicomponent nature of winds of low metallicity stars is characterised not only by the low density of driving ions, but also by lower mass-loss rate. (cs)
Title
  • On multicomponent effects in stellar winds of stars at extremely low metallicity
  • On multicomponent effects in stellar winds of stars at extremely low metallicity (en)
  • On multicomponent effects in stellar winds of stars at extremely low metallicity (cs)
skos:prefLabel
  • On multicomponent effects in stellar winds of stars at extremely low metallicity
  • On multicomponent effects in stellar winds of stars at extremely low metallicity (en)
  • On multicomponent effects in stellar winds of stars at extremely low metallicity (cs)
skos:notation
  • RIV/00216224:14310/03:00008001!RIV08-GA0-14310___
http://linked.open.../vavai/riv/strany
  • 713-718
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/01/0656), P(GA205/02/0445), Z(AV0Z1003909)
http://linked.open...iv/cisloPeriodika
  • 402
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
  • 619385
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/03:00008001
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars: mass-loss -- stars: early-type -- stars:abundances -- stars: winds; outflows (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [DEB8AF6EF2F1]
http://linked.open...i/riv/nazevZdroje
  • Astronomy and Astrophysics
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...v/svazekPeriodika
  • 35
http://linked.open...iv/tvurceVysledku
  • Krtička, Jiří
  • Kubát, Jiří
  • Owocki, Stanley P.
  • Brown, John C.
  • Galloway, Ross K.
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://localhost/t...ganizacniJednotka
  • 14310
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