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  • Recent calculations of multicomponent radiatively driven stellar winds of cool B stars showed that friction between individual components significantly lowers the terminal wind velocity. In addition, there is a large heating at the base of these winds caused by frictional and Gayley-Owocki heating. Such winds may be highly unstable resulting either in radiative-acoustic waves propagating both downstream and upstream or in unstable regions. Consequently, instabilities in the stellar wind influence the photospheric structure of these stars.
  • Recent calculations of multicomponent radiatively driven stellar winds of cool B stars showed that friction between individual components significantly lowers the terminal wind velocity. In addition, there is a large heating at the base of these winds caused by frictional and Gayley-Owocki heating. Such winds may be highly unstable resulting either in radiative-acoustic waves propagating both downstream and upstream or in unstable regions. Consequently, instabilities in the stellar wind influence the photospheric structure of these stars. (en)
  • Recent calculations of multicomponent radiatively driven stellar winds of cool B stars showed that friction between individual components significantly lowers the terminal wind velocity. In addition, there is a large heating at the base of these winds caused by frictional and Gayley-Owocki heating. Such winds may be highly unstable resulting either in radiative-acoustic waves propagating both downstream and upstream or in unstable regions. Consequently, instabilities in the stellar wind influence the photospheric structure of these stars. (cs)
Title
  • Instability Caused by a Multicomponent Nature of Radiatively-driven Stellar Winds
  • Instability Caused by a Multicomponent Nature of Radiatively-driven Stellar Winds (en)
  • Instability Caused by a Multicomponent Nature of Radiatively-driven Stellar Winds (cs)
skos:prefLabel
  • Instability Caused by a Multicomponent Nature of Radiatively-driven Stellar Winds
  • Instability Caused by a Multicomponent Nature of Radiatively-driven Stellar Winds (en)
  • Instability Caused by a Multicomponent Nature of Radiatively-driven Stellar Winds (cs)
skos:notation
  • RIV/00216224:14310/03:00008053!RIV08-GA0-14310___
http://linked.open.../vavai/riv/strany
  • 525-528
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/01/0656), P(GA205/02/0445)
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
  • 610656
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/03:00008053
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars: mass-loss; stars:early-type; hydrodynamics; instabilities; waves (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [193530A813D2]
http://linked.open...v/mistoKonaniAkce
  • Porto, Portugal
http://linked.open...i/riv/mistoVydani
  • Dordrecht, The Netherlands
http://linked.open...i/riv/nazevZdroje
  • Asteroseismology Across the HR Diagram
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
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
number of pages
http://purl.org/ne...btex#hasPublisher
  • Kluwer Academic Publishers
https://schema.org/isbn
  • 1-4020-1173-3
http://localhost/t...ganizacniJednotka
  • 14310
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