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

0534063 - ASÚ 2021 RIV FR eng J - Článek v odborném periodiku
Harmanec, P. - Lipták, J. - Koubský, Pavel - Božić, H. - Labadie-Bartz, J. - Šlechta, Miroslav - Yang, S. - Harmanec, A.
A new study of the spectroscopic binary 7 Vul with a Be star primary.
Astronomy & Astrophysics. Roč. 639, July (2020), č. článku A32. ISSN 0004-6361. E-ISSN 1432-0746
Institucionální podpora: RVO:67985815
Klíčová slova: spectroscopic * emission-line * fundamental parameters
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.803, rok: 2020
Způsob publikování: Omezený přístup
https://doi.org/10.1051/0004-6361/202037964

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, 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, 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 He i 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) M-circle dot(N) and (0.6 +/- 0.1) M-circle dot(N) fi. If the presence of a hot subdwarf is firmly confirmed, 7Vul might be identified as a rare object with a B4-B5 primary - all Be + hot subdwarf systems found so far contain B0-B3 primaries.
Trvalý link: http://hdl.handle.net/11104/0312280