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rdf:type
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Description
| - o And is one of the most frequently observed B estars, both in photometry and spectroscopy. It is a multiple system of at least four stars (a Be star, a close binary of spectral types B7 and B8, and an A star). For over a century, numerous observers report a highly variable spectrum, photometric changes, and a substantial range of radial velocity. The star has changed back and forth between a shell-type and a normal B-type star. The last emission phase started in 1992 and ended in 2000. Analysis of the dynamical spectra at spectral lines Mg II 4481 A and He I 6678 A and radial velocity curves shows that the two binary components can be resolved. We decomposed the triple star spectra and computed orbital parameters of the binary companion using the KOREL code for spectrum disentangling.
- o And is one of the most frequently observed B estars, both in photometry and spectroscopy. It is a multiple system of at least four stars (a Be star, a close binary of spectral types B7 and B8, and an A star). For over a century, numerous observers report a highly variable spectrum, photometric changes, and a substantial range of radial velocity. The star has changed back and forth between a shell-type and a normal B-type star. The last emission phase started in 1992 and ended in 2000. Analysis of the dynamical spectra at spectral lines Mg II 4481 A and He I 6678 A and radial velocity curves shows that the two binary components can be resolved. We decomposed the triple star spectra and computed orbital parameters of the binary companion using the KOREL code for spectrum disentangling. (en)
- o And – jedna z Be hvězd nejčastěji pozorovaných fotometricky i spektroskopicky – je systém nejméně čtyř hvězd (Be hvězdy, těsné dvojhvězdy typu B7 a B8 a A-hvězdy). Více než sto let jsou pozorovány velké změny svítivosti, radiálních rychlostí i spektra, které se několikrát změnilo z typu shell na normální typ B a zpět. Poslední emisní období hvězda prodělala v letech 1992 – 2000. Analýzou dynamických spekter v čárách g II 4481 A a He I 6678 A a křivky radiálních rychlostí se podařilo rozlišit složky dvojhvězdy. Pomocí programu KOREL na disentangling spekter jsme rozložili spektra trojitého systému a určili orbitální parametry dvojhvězdy. (cs)
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Title
| - Orbital parameters of the binary companion in o And using spectrum disentangling
- Orbital parameters of the binary companion in o And using spectrum disentangling (en)
- Orbitalni parametry dvojhvězdného průvodce o And získané metodou disentanglingu spekter (cs)
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skos:prefLabel
| - Orbital parameters of the binary companion in o And using spectrum disentangling
- Orbital parameters of the binary companion in o And using spectrum disentangling (en)
- Orbitalni parametry dvojhvězdného průvodce o And získané metodou disentanglingu spekter (cs)
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skos:notation
| - RIV/67985815:_____/05:00031699!RIV06-AV0-67985815
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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
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http://linked.open...iv/cisloPeriodika
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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/67985815:_____/05:00031699
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http://linked.open...riv/jazykVysledku
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http://linked.open.../riv/klicovaSlova
| - stars; binaries; spectroscopy; o And (en)
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http://linked.open.../riv/klicoveSlovo
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http://linked.open...odStatuVydavatele
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http://linked.open...ontrolniKodProRIV
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http://linked.open...i/riv/nazevZdroje
| - Astrophysics and Space Science
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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...UplatneniVysledku
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http://linked.open...v/svazekPeriodika
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http://linked.open...iv/tvurceVysledku
| - Hadrava, Petr
- Budovičová, Andrea
- Štefl, Stanislav
- Stahl, O.
- Rivinius, Th.
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http://linked.open...n/vavai/riv/zamer
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issn
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number of pages
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