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
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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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
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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
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