Počet záznamů: 1  

Relativistic apsidal motion in eccentric eclipsing binaries

  1. 1.
    0354432 - ASÚ 2011 RIV FR eng J - Článek v odborném periodiku
    Wolf, M. - Claret, L. - Kotková, Lenka - Kučáková, H. - Kocián, R. - Brát, L. - Svoboda, P. - Šmelcer, L.
    Relativistic apsidal motion in eccentric eclipsing binaries.
    Astronomy & Astrophysics. Roč. 509, January (2010), A18/1-A18/14. ISSN 0004-6361. E-ISSN 1432-0746
    Grant ostatní: GA ČR(CZ) GA205/04/2063; GA ČR(CZ) GA205/06/0217
    Výzkumný záměr: CEZ:AV0Z10030501
    Klíčová slova: binaries eclipsing
    Obor OECD: Astronomy (including astrophysics,space science)
    Impakt faktor: 4.410, rok: 2010

    As part of the long-term Ondrejov and Ostrava observational projects, we aim to measure precise times of minima for eccentric eclipsing binaries, needed for the accurate determination of apsidal motion, providing a suitable test of the effects of General Relativity. We confirm very long periods of apsidal motion for all systems. For BF Dra and V1094 Tau, we present the first apsidal-motion solution. The relativistic effects are dominant, representing up to 100% of the total observable apsidal-motion rate in several systems. The theoretical and observed values of the internal structure constant k(2) were compared for systems with lower relativistic contribution. Using the light-time effect solution, we predict a faint third component for V1094 Tau orbiting with a short period of about 8 years.
    Trvalý link: http://hdl.handle.net/11104/0193433

     
     
Počet záznamů: 1  

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