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  • There is evidence that at least some stars undergoing the Be phenomenon are single, almost critically rotating stars surrounded by viscous Keplerian disks. By combining our new stellar evolutionary tracks for critically rotating B-type stars with different masses and metallicities, with the parametrized expressions by Krtička et al. (2011) describing the properties of a stationary viscous Keplerian disk surrounding a star rotating at its breakup limit, we are able to explore for the first time how the properties of such a disk changes along the main sequence evolution of the star. The results we obtain can be relevant in the understanding of the formation and existence of Keplerian viscous decretion disks around rapidly rotating single Be stars.
  • There is evidence that at least some stars undergoing the Be phenomenon are single, almost critically rotating stars surrounded by viscous Keplerian disks. By combining our new stellar evolutionary tracks for critically rotating B-type stars with different masses and metallicities, with the parametrized expressions by Krtička et al. (2011) describing the properties of a stationary viscous Keplerian disk surrounding a star rotating at its breakup limit, we are able to explore for the first time how the properties of such a disk changes along the main sequence evolution of the star. The results we obtain can be relevant in the understanding of the formation and existence of Keplerian viscous decretion disks around rapidly rotating single Be stars. (en)
Title
  • Disks Surrounding Be stars: A Stellar Evolution Perspective
  • Disks Surrounding Be stars: A Stellar Evolution Perspective (en)
skos:prefLabel
  • Disks Surrounding Be stars: A Stellar Evolution Perspective
  • Disks Surrounding Be stars: A Stellar Evolution Perspective (en)
skos:notation
  • RIV/00216224:14310/12:00058608!RIV13-GA0-14310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/08/0003)
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
  • 131503
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/12:00058608
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • be stars disks (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [B58F5D73F398]
http://linked.open...v/mistoKonaniAkce
  • Foz do Iguacu, Brazilie
http://linked.open...i/riv/mistoVydani
  • San Francisco
http://linked.open...i/riv/nazevZdroje
  • Circumstellar Dynamics at High Resolution
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
  • Ekström, S.
  • Georgy, C.
  • Granada, A.
  • Meynet, G.
  • Owocki, S. P.
http://linked.open...vavai/riv/typAkce
http://linked.open...ain/vavai/riv/wos
  • 000314853500015
http://linked.open.../riv/zahajeniAkce
number of pages
http://purl.org/ne...btex#hasPublisher
  • Astronomical Society of the Pacific
https://schema.org/isbn
  • 9781583818107
http://localhost/t...ganizacniJednotka
  • 14310
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