About: Properties and nature of Be stars. 25. A new orbital solution and the nature of a peculiar emission-line binary upsilon Sagittarii     Goto   Sponge   NotDistinct   Permalink

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Description
  • Použitím nově získaných spektrálních data jsme odvodili pro tuto hvězdu nové orbitální elementy a křivku radiální rychlosti absorpce v čáře H alpha. Na základě detailní analýzy dostupných informací vylučujeme možnost vysvětlení pozorovaného chování modelem koronálního toku hmoty z jasnější složky a navrhujeme model pseudo-fotosféry opticky tlustého disku. (cs)
  • Using newly acquired spectral data we have derived the new orbital elements and RV curve of H alpha absorption of this star. Detailed analysis of available information rules out the explanation of observed behaviour by the model of coronal flow of matter from brighter component and suggests a model of pseudophotosphere of an optically thick disc.
  • Using newly acquired spectral data we have derived the new orbital elements and RV curve of H alpha absorption of this star. Detailed analysis of available information rules out the explanation of observed behaviour by the model of coronal flow of matter from brighter component and suggests a model of pseudophotosphere of an optically thick disc. (en)
Title
  • Properties and nature of Be stars. 25. A new orbital solution and the nature of a peculiar emission-line binary upsilon Sagittarii
  • Properties and nature of Be stars. 25. A new orbital solution and the nature of a peculiar emission-line binary upsilon Sagittarii (en)
  • Vlastnosti a povaha Be hvězd. 25. Nové orbitální řešení a povaha podivné dvojhvězdy (cs)
skos:prefLabel
  • Properties and nature of Be stars. 25. A new orbital solution and the nature of a peculiar emission-line binary upsilon Sagittarii
  • Properties and nature of Be stars. 25. A new orbital solution and the nature of a peculiar emission-line binary upsilon Sagittarii (en)
  • Vlastnosti a povaha Be hvězd. 25. Nové orbitální řešení a povaha podivné dvojhvězdy (cs)
skos:notation
  • RIV/67985815:_____/06:00099012!RIV08-AV0-67985815
http://linked.open.../vavai/riv/strany
  • 849;857
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/03/0788), P(GA205/06/0584), P(KSK2043105), V, Z(AV0Z10030501)
http://linked.open...iv/cisloPeriodika
  • 3
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
  • 495561
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/06:00099012
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars; emission-line; Be stars (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [C89E7C0D94C1]
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
  • 459
http://linked.open...iv/tvurceVysledku
  • Korčáková, Daniela
  • Škoda, Petr
  • Šlechta, Miroslav
  • Koubský, Pavel
  • Harmanec, P.
  • Yang, S.
  • Netolický, M.
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
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