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OGLE-LMC-ECL-09937: The Most Massive Algol-Type Binary System with a Mass Measurement Accurate to 2%

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00506338" target="_blank" >RIV/67985815:_____/17:00506338 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.32023/0001-5237/67.4.3" target="_blank" >https://doi.org/10.32023/0001-5237/67.4.3</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.32023/0001-5237/67.4.3" target="_blank" >10.32023/0001-5237/67.4.3</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    OGLE-LMC-ECL-09937: The Most Massive Algol-Type Binary System with a Mass Measurement Accurate to 2%

  • Original language description

    This paper presents a detailed analysis of the light and radial velocity curves of the semi-detached eclipsing binary system OGLE-LMC-ECL-09937. The system is composed of a hot, massive and luminous primary star of a late-O spectral type, and a more evolved, but less massive and luminous secondary, implying an Algol-type system that underwent a mass transfer episode. We derive masses of 21.04 +/- 0.34 M-circle dot and 7.61 +/- 0.09 M-circle dot and radii of 9.93 +/- 0.06 R-circle dot and 9.18 +/- 0.04 R-circle dot, for the primary and the secondary component, respectively, which make it the most massive known Algol-type system with masses and radii of the components measured with < 2% accuracy. Consequently, the parameters of OGLE-LMC-ECL-09937 provide an important contribution to the sparsely populated high-mass end of the stellar mass distribution, and an interesting object for stellar evolution studies, being a possible progenitor of a binary system composed of two neutron stars.

  • 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

    2017

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Acta Astronomica

  • ISSN

    0001-5237

  • e-ISSN

  • Volume of the periodical

    67

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    PL - POLAND

  • Number of pages

    16

  • Pages from-to

    329-344

  • UT code for WoS article

    000423282900003

  • EID of the result in the Scopus database