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”

Eclipsing Binaries Within Visual Ones: Prospects of Combined Solution

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10129495" target="_blank" >RIV/00216208:11320/12:10129495 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921311027384" target="_blank" >http://dx.doi.org/10.1017/S1743921311027384</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921311027384" target="_blank" >10.1017/S1743921311027384</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Eclipsing Binaries Within Visual Ones: Prospects of Combined Solution

  • Original language description

    The study of eclipsing binaries as members of multiple systems can provide us important information about their origin, evolution, mutual inclination of the orbits, independent distance and mass determination, as well as the stellar multiplicity in general. We are carrying out a long-term photometric monitoring of several eclipsing binaries within the visual multiples and, besides the complete light curves, we are trying to detect the period changes due to the orbital motion around a common barycenter.Systems like DN UMa, V819 Her, LO Hya, or VW Cep are typical examples of eclipsing binaries orbiting around the barycenter of the multiple system, while their respective periods are on the order of years or decades. However, the expected period variationis only hardly detectable and there is still uncertainty about which of the components is the eclipsing one. Precise spectroscopy would be of great benefit, but detecting the changes in the gamma velocity is still problematic, and spectr

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • 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)

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS

  • ISBN

    978-1-107-01982-9

  • ISSN

    1743-9213

  • e-ISSN

  • Number of pages

    2

  • Pages from-to

    207-208

  • Publisher name

    CAMBRIDGE UNIV PRESS

  • Place of publication

    CAMBRIDGE

  • Event location

    Tatranska Lominica, SLOVAKIA

  • Event date

    Jul 18, 2011

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000309244400062