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rdf:type
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Description
| - 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)
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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)
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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)
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skos:notation
| - RIV/00216224:14310/03:00008053!RIV08-GA0-14310___
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http://linked.open.../vavai/riv/strany
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http://linked.open...avai/riv/aktivita
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http://linked.open...avai/riv/aktivity
| - P(GA205/01/0656), P(GA205/02/0445)
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http://linked.open...vai/riv/dodaniDat
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http://linked.open...aciTvurceVysledku
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http://linked.open.../riv/druhVysledku
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http://linked.open...iv/duvernostUdaju
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http://linked.open...titaPredkladatele
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http://linked.open...dnocenehoVysledku
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http://linked.open...ai/riv/idVysledku
| - RIV/00216224:14310/03:00008053
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http://linked.open...riv/jazykVysledku
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http://linked.open.../riv/klicovaSlova
| - stars: mass-loss; stars:early-type; hydrodynamics; instabilities; waves (en)
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http://linked.open.../riv/klicoveSlovo
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http://linked.open...ontrolniKodProRIV
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http://linked.open...v/mistoKonaniAkce
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http://linked.open...i/riv/mistoVydani
| - Dordrecht, The Netherlands
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http://linked.open...i/riv/nazevZdroje
| - Asteroseismology Across the HR Diagram
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http://linked.open...in/vavai/riv/obor
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http://linked.open...ichTvurcuVysledku
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http://linked.open...cetTvurcuVysledku
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http://linked.open...vavai/riv/projekt
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http://linked.open...UplatneniVysledku
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http://linked.open...iv/tvurceVysledku
| - Krtička, Jiří
- Kubát, Jiří
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http://linked.open...vavai/riv/typAkce
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http://linked.open.../riv/zahajeniAkce
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number of pages
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http://purl.org/ne...btex#hasPublisher
| - Kluwer Academic Publishers
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https://schema.org/isbn
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http://localhost/t...ganizacniJednotka
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