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

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00534063" target="_blank" >RIV/67985815:_____/20:00534063 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1051/0004-6361/202037964" target="_blank" >https://doi.org/10.1051/0004-6361/202037964</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202037964" target="_blank" >10.1051/0004-6361/202037964</a>

Alternative languages

  • 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, 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.

  • Czech name

  • Czech description

Classification

  • 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)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    639

  • Issue of the periodical within the volume

    July

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    15

  • Pages from-to

    A32

  • UT code for WoS article

    000549961400006

  • EID of the result in the Scopus database

    2-s2.0-85087915586