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Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10129571" target="_blank" >RIV/00216208:11320/12:10129571 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00388462 RIV/67985815:_____/13:00421152 RIV/00216208:11320/13:10173968 RIV/00216224:14310/13:00107092

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201117210" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201117210</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201117210" target="_blank" >10.1051/0004-6361/201117210</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon

  • Original language description

    We present results of nearly six years of spectroscopic observations of the B[e] star V2028 Cyg. The presence of the cold-type absorption lines combined with a hot-type spectrum indicate the binarity of this object. Since B[e] stars are embedded in an extended envelope, the usage of common stellar atmosphere models for the analysis is quite inappropriate. Therefore, we focus on the analysis of the long-term spectral line variations in order to determine the nature of this object. We present the time dependences of the equivalent width and radial velocities of the Ha line, [O I] 6300 angstrom, Fe II 6427, 6433, and 6456 angstrom lines. The bisector variations and line intensities are shown for the Ha line. The radial velocities are also measured for theabsorption lines of the K component. No periodic variation is found. The observed data show correlations between the measured quantities, which can be used in future modelling.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    542

  • Issue of the periodical within the volume

    červen

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    6

  • Pages from-to

  • UT code for WoS article

    000305803300007

  • EID of the result in the Scopus database