About: Spectroscopic study of the extremely fast rotating star 44 Geminorum

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An Entity of Type : http://linked.opendata.cz/ontology/domain/vavai/Vysledek, within Data Space : linked.opendata.cz associated with source document(s)

Attributes	Values
rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
Description	Stars with extremely fast rotation represent interesting challenge to modern understanding of the stellar evolution. The reasons why such a spin-up process should occur during the evolution to otherwise normal star are still not well understood. Already in the beginning of the XX century Otto Struve proposed that fast rotation of the group of stars spectroscopically classified as Be could be the main reason for the formation of observed disks of circumstellar material around them. This circumstellar material is responsible for the emission lines observed in the spectrum of Be-stars as well as for the whole complex of spectral and photometrical patterns called in general Be-phenomenon. Stars with extremely fast rotation represent interesting challenge to modern understanding of the stellar evolution. The reasons why such a spin-up process should occur during the evolution to otherwise normal star are still not well understood. Already in the beginning of the XX century Otto Struve proposed that fast rotation of the group of stars spectroscopically classified as Be could be the main reason for the formation of observed disks of circumstellar material around them. This circumstellar material is responsible for the emission lines observed in the spectrum of Be-stars as well as for the whole complex of spectral and photometrical patterns called in general Be-phenomenon. (en)
Title	Spectroscopic study of the extremely fast rotating star 44 Geminorum Spectroscopic study of the extremely fast rotating star 44 Geminorum (en)
skos:prefLabel	Spectroscopic study of the extremely fast rotating star 44 Geminorum Spectroscopic study of the extremely fast rotating star 44 Geminorum (en)
skos:notation	RIV/67985815:_____/12:00388470!RIV13-GA0-67985815
http://linked.open...avai/riv/aktivita	I P
http://linked.open...avai/riv/aktivity	I, P(GAP209/10/0967), P(IAA300030908), P(IAA301630901)
http://linked.open...iv/cisloPeriodika	12012
http://linked.open...vai/riv/dodaniDat	2013
http://linked.open...aciTvurceVysledku	Kawka, Adela Kubát, Jiří Németh, Péter Vennes, Stephane Kraus, Michaela
http://linked.open.../riv/druhVysledku	J - Článek v odborném periodiku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Astronomický ústav AV ČR, v. v. i.
http://linked.open...dnocenehoVysledku	170379
http://linked.open...ai/riv/idVysledku	RIV/67985815:_____/12:00388470
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	Be stars; emission line; fundamental parameter (en)
http://linked.open.../riv/klicoveSlovo	Be stars emission line fundamental parameter
http://linked.open...odStatuVydavatele	BG - Bulharská republika
http://linked.open...ontrolniKodProRIV	[7AE6716F71F0]
http://linked.open...i/riv/nazevZdroje	Bulgarian astronomical journal
http://linked.open...in/vavai/riv/obor	BN
http://linked.open...ichTvurcuVysledku	5 (xsd:int)
http://linked.open...cetTvurcuVysledku	7 (xsd:int)
http://linked.open...vavai/riv/projekt	Properties of the white dwarf population and their planetary connection Spectroscopy and Numerical Modeling of Stellar Atmospheres Spectral energy distribution of hot stars and its variability
http://linked.open...UplatneniVysledku	2012
http://linked.open...v/svazekPeriodika	18
http://linked.open...iv/tvurceVysledku	Kawka, Adela Németh, Péter Vennes, Stephane Kraus, Michaela Kubát, Jiří Iliev, L. Borisov, G.
issn	1313-2709
number of pages	9 (xsd:int)

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