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Apsidal motion and a light curve solution for eighteen SMC eccentric eclipsing binaries

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10286183" target="_blank" >RIV/00216208:11320/14:10286183 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216224:14310/14:00078450

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201424273" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201424273</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201424273" target="_blank" >10.1051/0004-6361/201424273</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Apsidal motion and a light curve solution for eighteen SMC eccentric eclipsing binaries

  • Original language description

    Aims. The Danish 1.54-meter telescope at the La Silla observatory was used for photometric monitoring of selected eccentric eclipsing binaries located in the Small Magellanic Cloud. The new times of minima were derived for these systems, which are neededfor accurate determination of the apsidal motion. Moreover, many new times of minima were derived from the photometric databases OGLE and MACHO. Eighteen early-type eccentric-orbit eclipsing binaries were studied. Methods. Their O-C diagrams of minima timings were analysed and the parameters of the apsidal motion were obtained. The light curves of these eighteen binaries were analysed using the program PHOEBE, giving the light curve parameters. For several systems, the additional third light also was detected. Results. We derived for the first time and significantly improved the relatively short periods of apsidal motion from 19 to 142 years for these systems. The relativistic effects are weak, up to 10% of the total apsidal motion rat

  • 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

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

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

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

    572

  • Issue of the periodical within the volume

    prosinec

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    8

  • Pages from-to

  • UT code for WoS article

    000346101700091

  • EID of the result in the Scopus database