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GK Bootis and AE Fornacis: two low-mass eclipsing binaries with dwarf companions

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10123641" target="_blank" >RIV/00216208:11320/12:10123641 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/" target="_blank" >http://dx.doi.org/</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201117417" target="_blank" >10.1051/0004-6361/201117417</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    GK Bootis and AE Fornacis: two low-mass eclipsing binaries with dwarf companions

  • Original language description

    Context. A study of late-type low-mass eclipsing binaries provides us with important information about the most common stars in the Universe. Aims. We obtain the first light curves and perform period analyses of two neglected eclipsing binaries GK Boo and AE For to reveal their basic physical properties. Methods. We performed both a period analysis of the times of the minima and a BVR light curve analysis. Many new times of minima for both the systems were derived and collected from the data obtained byautomatic and robotic telescopes. This allowed us to study the long-term period changes in these systems for the first time. From the light curve analysis, we derived the first rough estimates of the physical properties of these systems. Results. We find that the analyzed systems are somewhat similar to each other. Both contain low-mass components of similar types, both are close to the Sun, both have short orbital period, and both contain another low-mass companions on longer orbits of

  • 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

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2012

  • 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

    537

  • Issue of the periodical within the volume

    leden

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    8

  • Pages from-to

  • UT code for WoS article

    000300416800109

  • EID of the result in the Scopus database