All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Possible substellar companions in low-mass eclipsing binaries: GU Bootis and YY Geminorum

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F18%3AA0000356" target="_blank" >RIV/47813059:19240/18:A0000356 - isvavai.cz</a>

  • Alternative codes found

    RIV/00371912:_____/18:N0000001

  • Result on the web

    <a href="https://www.aanda.org/articles/aa/abs/2018/12/aa33708-18/aa33708-18.html" target="_blank" >https://www.aanda.org/articles/aa/abs/2018/12/aa33708-18/aa33708-18.html</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201833708" target="_blank" >10.1051/0004-6361/201833708</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Possible substellar companions in low-mass eclipsing binaries: GU Bootis and YY Geminorum

  • Original language description

    We present the next results of our long-term observational project to analyze the variations in the orbital periods of low-mass eclipsing binaries. About 70 new precise mid-eclipse times recorded with a CCD were obtained for two eclipsing binaries with short orbital periods: GU Boo (P = 0.^{d}49) and YY Gem (0.^{d}81). Observed-minus-calculated diagrams of the stars were analyzed using all reliable timings, and new parameters of the light-time effect were obtained. We derived for the first time or improved the short orbital periods of possible third bodies of 11 and 54 years for these low-mass binaries, respectively. We calculated that the minimum masses of the third components are close to 50 M_{Jup}, which corresponds to the mass of brown dwarfs. The multiplicity of these systems also plays an important role in the precise determination of their physical parameters.

  • 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

    2018

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    620

  • Issue of the periodical within the volume

    December

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    7

  • Pages from-to

    „A72-1“-„A72-7“

  • UT code for WoS article

    000452389400002

  • EID of the result in the Scopus database

    2-s2.0-85058064404