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The two eccentric eclipsing binaries in multiple systems: V539 Arae and V335 Serpentis

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00555881" target="_blank" >RIV/67985815:_____/22:00555881 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/22:00555881 RIV/00216208:11320/22:10455230 RIV/00216224:14310/22:00125358 RIV/47813059:19630/22:A0000224

  • Result on the web

    <a href="https://doi.org/10.1016/j.newast.2021.101708" target="_blank" >https://doi.org/10.1016/j.newast.2021.101708</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.newast.2021.101708" target="_blank" >10.1016/j.newast.2021.101708</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The two eccentric eclipsing binaries in multiple systems: V539 Arae and V335 Serpentis

  • Original language description

    We present new results of our long-term observational project to analyze the variations of the orbital period for early-type eccentric eclipsing binaries. Altogether 77 new mid-eclipse times were measured or derived for two eclipsing binaries, namely V539 Ara and V335 Ser. Based on current O - C diagrams, we found in both systems that times of minima besides the typical apsidal motion show additional cyclical changes likely caused by the third or fourth bodies orbiting the eclipsing pair. The improved periods of apsidal motion are 155 and 1080 years, respectively. For the first time we propose a third and fourth body orbiting V539 Ara, stellar companions in a hierarchical system with a minimal mass of 0.41 and 1.74 Ms. In V355 Ser we found a possible third body with a mass of 0.18 Ms orbiting this eclipsing pair. The third- and fourth-body orbital periods are relatively short: 29 and 57 yr in case of V539 Ara, and 25 yr for V335 Ser.

  • 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

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

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    New Astronomy

  • ISSN

    1384-1076

  • e-ISSN

    1384-1092

  • Volume of the periodical

    92

  • Issue of the periodical within the volume

    April

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    6

  • Pages from-to

    101708

  • UT code for WoS article

    000707225600002

  • EID of the result in the Scopus database

    2-s2.0-85117145899