J 2004

Apsidal motion in eccentric eclipsing binaries: V871 Aql, V345 Lac, V401 Lac and CR Sct

WOLF, Marek; Petr HARMANEC; Lenka ŠAROUNOVÁ; Miloslav ZEJDA; Hrvoje BOŽIČ et. al.

Basic information

Original name

Apsidal motion in eccentric eclipsing binaries: V871 Aql, V345 Lac, V401 Lac and CR Sct

Name in Czech

Apsidální pohyb v excentrických dvojhvězdách: V871 Aql, V345 Lac, V401 Lac a CR Sct

Authors

WOLF, Marek; Petr HARMANEC; Lenka ŠAROUNOVÁ; Miloslav ZEJDA; Hrvoje BOŽIČ; Kamil HORNOCH; V. S. KOZYREVA; T. HYNEK and Lukáš KRÁL

Edition

Astronomy and Astrophysics, Heidelberg, Springer-Verlag, 2004, 0004-6361

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

Germany

Confidentiality degree

is not subject to a state or trade secret

Impact factor

Impact factor: 3.694

RIV identification code

RIV/00216224:14310/04:00020165

Organization unit

Faculty of Science

UT WoS

000222606200023

Keywords in English

eclipsing binary; apsidal motion;V871 Aql; V345 Lac; V401 Lac; CR Sct

Tags

International impact, Reviewed
Changed: 29/3/2010 10:17, doc. RNDr. Miloslav Zejda, Ph.D.

Abstract

In the original language

About thirty new times of minimum light recorded with photoelectric or CCD photometers were obtained for several little studied eccentric-orbit eclipsing binaries V871 Aql (P=3.0 d, e=0.13), V345 Lac ( 7.5 d, 0.46), V401 Lac ( 2.0 d, 0.16) and CR Sct ( 4.2 d, 0.09). Their O-C diagrams were analyzed using all reliable timings found in the literature and in all cases an apsidal motion was either discovered or confirmed. The new values for the elements of the apsidal motion were derived. We find periods of apsidal motion of about 255, 7000, 79.4 and 4400 years for V871 Aql, V345 Lac, V401 Lac and CR Sct, respectively. Partly based on photoelectric observations secured at the Hvar Observatory, Zagreb University, Croatia.

In Czech

Přibližně 30 nových okamžiků minim bylo získáno fotoelektrickým fotometrem nebo CCD pro několik málo studovaných excentrických dvojhvězd V871 Aql, V345 Lac, V401 Lac a CR Sct. Použitím všech dostupných okmažiků minim byly analyzovány jejich O-C diagramy a ve všech případech byl objeven nebo potvrzen apsidální pohyb. Byly určeny nové elementy apsidálního pohybu s periodami 255, 7000, 79.4 a 4400 let pro V871 Aql, V345 Lac, V401 Lac a CR Sct.

Links

GA205/04/2063, research and development project
Name: Fotometrický výzkum zákrytových dvojhvězd
Investor: Czech Science Foundation