0124794 - ASU-R 20010047 RIV FR eng J - Článek v odborném periodiku
Lehmann, H. - Harmanec, Petr - Aerts, C. - Božić, H. - Eenens, P. - Hildebrandt, G. - Holmgren, D. - Mathias, P. - Scholz, G. - Šlechta, Miroslav - Yang, S.
A new analysis of the radial velocity variations of the eclipsing and spectroscopic binary EN Lacertae.
Astronomy & Astrophysics. Roč. 367, č. 1 (2001), s. 236-249. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA AV ČR IAA3003805
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: stars binaries * spectroscopic * oscillations
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 2.790, rok: 2000

The accuracy of the orbital solution has been substantially improved after the observed RV changes were properly prewhitened for the short-term oscillations. The analysis of RV scatter gives some indication of a sharp increase of this scatter when the stars are approaching periastron. Since this could be a signature of forced oscillations.
Trvalý link: http://hdl.handle.net/11104/0023053