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HD 165246: an early-type binary with a low mass ratio

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10174137" target="_blank" >RIV/00216208:11320/13:10174137 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201220388" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201220388</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201220388" target="_blank" >10.1051/0004-6361/201220388</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    HD 165246: an early-type binary with a low mass ratio

  • Original language description

    Analyses of 13 FEROS spectra from the ESO archive and 617 V-band photometric observations from the ASAS3 database allowed us to demonstrate that HD 165246 is a double-lined spectroscopic binary. As an earlier finding revealed, HD 165246 is also an eclipsing system. We were able to derive consistent orbital and light-curve solutions and all basic physical properties of the system. The period of this O8V + B7V binary is 4(d).592706 and the semiamplitudes of the radial-velocity curves are K-1 = 55.5 km s(-1) and K-2 = 321 km s(-1). As the mass ratio is small (0.173), the secondary lines cannot be seen directly in the spectra; however the application of spectral disentangling allowed us to detect weak Balmer and He I lines of the secondary component. The primary component rotates with a high projected velocity of v sin i = 243 km s(-1). A combined radial-velocity and light-curve solution led to the component masses and radii expected for the young stars of the given spectral types. Due to

  • 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

    <a href="/en/project/GAP209%2F10%2F0715" target="_blank" >GAP209/10/0715: Accurate physical properties of hot stars based on binary and multiple star studies</a><br>

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2013

  • 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

    550

  • Issue of the periodical within the volume

    únor

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    7

  • Pages from-to

  • UT code for WoS article

    000314879700002

  • EID of the result in the Scopus database