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Statements

Subject Item
n2:RIV%2F00216224%3A14310%2F05%3A00013305%21RIV10-MSM-14310___
rdf:type
skos:Concept n21:Vysledek
dcterms:description
We calculated spectral energy distribution of the helium strong chemically peculiar star HD 37776 using adequate model atmospheres. We show that the chemical peculiarity influences the stellar energy distribution. Consequently, spots of peculiar chemical composition on the surface of a rotating star may cause detectable light variations of the star. However, the observed light variations are not likely caused by an uneven surface distribution of helium, but may be due to spots of metals (mainly carbon). We calculated spectral energy distribution of the helium strong chemically peculiar star HD 37776 using adequate model atmospheres. We show that the chemical peculiarity influences the stellar energy distribution. Consequently, spots of peculiar chemical composition on the surface of a rotating star may cause detectable light variations of the star. However, the observed light variations are not likely caused by an uneven surface distribution of helium, but may be due to spots of metals (mainly carbon).
dcterms:title
The Nature of Light Variations of the He-Strong CP Star HD 37776 The Nature of Light Variations of the He-Strong CP Star HD 37776
skos:prefLabel
The Nature of Light Variations of the He-Strong CP Star HD 37776 The Nature of Light Variations of the He-Strong CP Star HD 37776
skos:notation
RIV/00216224:14310/05:00013305!RIV10-MSM-14310___
n3:aktivita
n9:P
n3:aktivity
P(GA205/04/1267), P(GP205/03/D020), P(ME 128)
n3:dodaniDat
n8:2010
n3:domaciTvurceVysledku
n10:5322324 n10:4066790 n10:2439549 n10:4156722
n3:druhVysledku
n16:D
n3:duvernostUdaju
n6:S
n3:entitaPredkladatele
n4:predkladatel
n3:idSjednocenehoVysledku
532109
n3:idVysledku
RIV/00216224:14310/05:00013305
n3:jazykVysledku
n15:eng
n3:klicovaSlova
stars: atmospheres; stars: chemically peculiar; stars: early-type; stars: variables: other; object: HD 37776
n3:klicoveSlovo
n12:stars%3A%20chemically%20peculiar n12:stars%3A%20atmospheres n12:stars%3A%20variables%3A%20other n12:stars%3A%20early-type n12:object%3A%20HD%2037776
n3:kontrolniKodProRIV
[10ACC719D337]
n3:mistoKonaniAkce
Sapporo, Japonsko
n3:mistoVydani
San Francisco, USA
n3:nazevZdroje
Active OB-Stars: Laboratories For Stellar and Circumstellar Physics
n3:obor
n11:BN
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
4
n3:projekt
n14:GA205%2F04%2F1267 n14:ME%20128 n14:GP205%2F03%2FD020
n3:rokUplatneniVysledku
n8:2005
n3:tvurceVysledku
Žižnovský, Jozef Krtička, Jiří Zverko, Juraj Mikulášek, Zdeněk
n3:typAkce
n17:WRD
n3:zahajeniAkce
2005-01-01+01:00
s:numberOfPages
3
n7:hasPublisher
Astronomical Society of the Pacific
n18:isbn
978-1-58381-229-7
n19:organizacniJednotka
14310