A new study of the spectroscopic binary 7 Vul with a Be star primary

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F20%3A10422782" target="_blank" >RIV/00216208:11320/20:10422782 - isvavai.cz</a>
Result on the web
<a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=2-CK.wEByM" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=2-CK.wEByM</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202037964" target="_blank" >10.1051/0004-6361/202037964</a>

Result language
angličtina
Original language name
A new study of the spectroscopic binary 7 Vul with a Be star primary
Original language description
We confirmed the binary nature of the Be star 7 Vul, derived a more accurate spectroscopic orbit with an orbital period of 69(.)(d)4212 +/- 0(.)(d)0034 69 . d 4212 +/- 0 . d 0034 , and improved the knowledge of the basic physical elements of the system. Analyzing available photometry and the strength of the H alpha emission, we also document the long-term spectral variations of the Be primary. In addition, we confirmed rapid light changes with a period of 0(.)(d)5592 0 . d 5592 , which is comparable to the expected rotational period of the Be primary, but note that its amplitude and possibly its period vary with time. We were able to disentangle only the HeI 6678 angstrom line of the secondary, which could support our tentative conclusion that the secondary appears to be a hot subdwarf. A search for this object in high-dispersion far-UV spectra could provide confirmation. Probable masses of the binary components are (6 +/- 1) ?(N)(circle dot) M circle dot N and (0.6 +/- 0.1) ?(N)(circle dot) M circle dot N . If the presence of a hot subdwarf is firmly confirmed, 7 Vul might be identified as a rare object with a B4-B5 primary; all Be + hot subdwarf systems found so far contain B0-B3 primaries.
Czech name
—
Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GA19-01995S" target="_blank" >GA19-01995S: Studying long-term variability and duplicity of individual classical as well as other Be stars with multi-technique observations</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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