About: NLTE model atmospheres of irradiated stars in B binaries.     Goto   Sponge   NotDistinct   Permalink

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  • Model atmospheres of B stars irradiated by their companion are calculated using our model atmosphere computer code under the assumption of hydrostatic, radiative, and statistical equilibrium. The external source of radiation is able to change the temperature structure of the outer atmospheric layers of B stars significantly.
  • Model atmospheres of B stars irradiated by their companion are calculated using our model atmosphere computer code under the assumption of hydrostatic, radiative, and statistical equilibrium. The external source of radiation is able to change the temperature structure of the outer atmospheric layers of B stars significantly. (en)
Title
  • NLTE model atmospheres of irradiated stars in B binaries.
  • NLTE model atmospheres of irradiated stars in B binaries. (en)
skos:prefLabel
  • NLTE model atmospheres of irradiated stars in B binaries.
  • NLTE model atmospheres of irradiated stars in B binaries. (en)
skos:notation
  • RIV/67985815:_____/00:01000153!RIV/2003/AV0/A01003/N
http://linked.open.../vavai/riv/strany
  • 705;708
http://linked.open...avai/riv/aktivita
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  • Z(AV0Z1003909)
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  • 719311
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  • RIV/67985815:_____/00:01000153
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  • N/A (en)
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  • [F314034CA177]
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  • Alicante [ES]
http://linked.open...i/riv/mistoVydani
  • San Francisco
http://linked.open...i/riv/nazevZdroje
  • The Be phenomenon in early-type stars.
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...ocetUcastnikuAkce
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  • Kubát, Jiří
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  • Astronomical Society of the Pacific
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