Number of the records: 1

On the nature of the Be star HR 7409 (7 Vul)

SYSNO ASEP	0367852
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	On the nature of the Be star HR 7409 (7 Vul)
Author(s)	Vennes, Stephane (ASU-R)_{ORCID, RID} Kawka, Adela (ASU-R)_{ORCID, RID} Jonić, S. (RS) Pirković, I. (RS) Iliev, I. (BG) Kubát, Jiří (ASU-R)_{RID, ORCID} Šlechta, Miroslav (ASU-R)_{RID, ORCID} Németh, Péter (ASU-R)_ORCID Kraus, Michaela (ASU-R)_{RID, ORCID}
Source Title	Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711 Roč. 413, č. 4 (2011), s. 2760-2766
Number of pages	7 s.
Language	eng - English
Country	GB - United Kingdom
Keywords	Be stars ; emission-line ; individual star HR 7409
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA300030908 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	IAA301630901 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	GAP209/10/0967 GA ČR - Czech Science Foundation (CSF)
	LC06014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000290819900038
DOI	10.1111/j.1365-2966.2011.18350.x
Annotation	HR 7409 (7 Vul) is a newly identified Be star, possibly part of the Gould Belt, and is the massive component of a 69-d spectroscopic binary. The binary parameters and properties of the Be star measured using high-dispersion spectra obtained at Ondřejov Observatory and at Rozhen Observatory imply the presence of a low-mass companion.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2012

Number of the records: 1