This HTML5 document contains 40 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
n13http://linked.opendata.cz/ontology/domain/vavai/riv/typAkce/
dctermshttp://purl.org/dc/terms/
n18http://purl.org/net/nknouf/ns/bibtex#
n17http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n7http://linked.opendata.cz/ontology/domain/vavai/
n19http://linked.opendata.cz/resource/domain/vavai/zamer/
shttp://schema.org/
skoshttp://www.w3.org/2004/02/skos/core#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n16http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n6http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n10http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F67985815%3A_____%2F00%3A01000151%21RIV%2F2003%2FAV0%2FA01003%2FN/
n12http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n4http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n15http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n9http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n11http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F00%3A01000151%21RIV%2F2003%2FAV0%2FA01003%2FN
rdf:type
n7:Vysledek skos:Concept
dcterms:description
The Be binary star CX Dra has been observed with the IUE satellite over a period of 14 years. After processing the quotient flux spectra of the Al III and Si IV lines show very complicated behaviour. The most important features are the violet shifted components in these lines which show very negative velocities in a particular phase interval. The Be binary star CX Dra has been observed with the IUE satellite over a period of 14 years. After processing the quotient flux spectra of the Al III and Si IV lines show very complicated behaviour. The most important features are the violet shifted components in these lines which show very negative velocities in a particular phase interval.
dcterms:title
IUE spectra of Be star CX Dra: evidence for Winds. IUE spectra of Be star CX Dra: evidence for Winds.
skos:prefLabel
IUE spectra of Be star CX Dra: evidence for Winds. IUE spectra of Be star CX Dra: evidence for Winds.
skos:notation
RIV/67985815:_____/00:01000151!RIV/2003/AV0/A01003/N
n3:strany
573;576
n3:aktivita
n4:Z
n3:aktivity
Z(AV0Z1003909)
n3:dodaniDat
n11:2003
n3:domaciTvurceVysledku
n17:8647623 n17:3561585
n3:druhVysledku
n15:D
n3:duvernostUdaju
n6:S
n3:entitaPredkladatele
n10:predkladatel
n3:idSjednocenehoVysledku
714239
n3:idVysledku
RIV/67985815:_____/00:01000151
n3:jazykVysledku
n12:eng
n3:klicovaSlova
N/A
n3:klicoveSlovo
n16:N%2FA
n3:kontrolniKodProRIV
[0A9D51917AEB]
n3:mistoKonaniAkce
Alicante [ES]
n3:mistoVydani
San Francisco
n3:nazevZdroje
The Be phenomenon in early-type stars.
n3:obor
n9:BN
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
2
n3:pocetUcastnikuAkce
0
n3:pocetZahranicnichUcastnikuAkce
0
n3:rokUplatneniVysledku
n11:2000
n3:tvurceVysledku
Koubský, Pavel Škoda, Petr
n3:typAkce
n13:WRD
n3:zahajeniAkce
1999-06-28+02:00
n3:zamer
n19:AV0Z1003909
s:numberOfPages
4
n18:hasPublisher
Astronomical Society of the Pacific