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HD 152246: a new high-mass triple system and its basic properties

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10287024" target="_blank" >RIV/00216208:11320/14:10287024 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201424382" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201424382</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201424382" target="_blank" >10.1051/0004-6361/201424382</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    HD 152246: a new high-mass triple system and its basic properties

  • Original language description

    Analyses of multi-epoch, high-resolution (R similar to 50 000) optical spectra of the O-type star HD 152246 (09 IV according to the most recent classification), complemented by a limited number of earlier published radial velocities, led to the finding that the object is a hierarchical triple system, where a close inner pair (Ba-Bb) with a slightly eccentric orbit (e = 0.11) and a period of 6.0049 revolves in a 470-day highly eccentric orbit (e = 0.865) with another massive and brighter component A. Themass ratio of the inner system must be low since we were unable to find any traces of the secondary spectrum. The mass ratio A/(Ba+Bb) is 0.89. The outer system has recently been resolved using long-baseline interferometry on three occasions. The interferometry confirms the spectroscopic results and specifies elements of the system. Our orbital solutions, including the combined radial-velocity and interferometric solution indicate an orbital inclination of the outer orbit of 112 and ste

  • 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)<br>S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2014

  • 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

    568

  • Issue of the periodical within the volume

    srpen

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    9

  • Pages from-to

  • UT code for WoS article

    000341185900131

  • EID of the result in the Scopus database