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On the nature of the Be star HR 7409 (7 Vul)
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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, ORCIDSource Title Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711
Roč. 413, č. 4 (2011), s. 2760-2766Number 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 https://doi.org/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 Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2012
Number of the records: 1