About: Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E     Goto   Sponge   NotDistinct   Permalink

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  • We study the possibility of the helium decoupling in the stellar wind of sigma Ori E. To obtain reliable wind parameters for this star we first calculate NLTE wind model and derive wind mass-loss rate and terminal velocity. Using corresponding force multipliers we study the possibility of helium decoupling. We find that helium decoupling is not possible for realistic values of helium charge (calculated from NLTE wind models). Helium decoupling only seems possible for a very low helium charge. The reason for this behavior is the strong coupling between helium and hydrogen. We also find that frictional heating becomes important in the outer parts of the wind of sigma Ori E due to the collisions between some heavier elements and the passive components - hydrogen and helium. For a metallicity ten times lower than the solar one, both hydrogen and helium decouple from the metals and may fall back onto the stellar surface.
  • We study the possibility of the helium decoupling in the stellar wind of sigma Ori E. To obtain reliable wind parameters for this star we first calculate NLTE wind model and derive wind mass-loss rate and terminal velocity. Using corresponding force multipliers we study the possibility of helium decoupling. We find that helium decoupling is not possible for realistic values of helium charge (calculated from NLTE wind models). Helium decoupling only seems possible for a very low helium charge. The reason for this behavior is the strong coupling between helium and hydrogen. We also find that frictional heating becomes important in the outer parts of the wind of sigma Ori E due to the collisions between some heavier elements and the passive components - hydrogen and helium. For a metallicity ten times lower than the solar one, both hydrogen and helium decouple from the metals and may fall back onto the stellar surface. (en)
Title
  • Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E
  • Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E (en)
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  • Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E
  • Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E (en)
skos:notation
  • RIV/00216224:14310/06:00016004!RIV10-GA0-14310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/04/1267), P(GP205/03/D020), Z(AV0Z10030501)
http://linked.open...iv/cisloPeriodika
  • 1
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
  • 487232
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/06:00016004
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars: winds outflows - stars: mass-loss - stars: early-type - hydrodynamics - stars: chemically peculiar (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [2FFFB20BA988]
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
  • 460
http://linked.open...iv/tvurceVysledku
  • Krtička, Jiří
  • Kubát, Jiří
  • Groote, Detlef
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://localhost/t...ganizacniJednotka
  • 14310
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