Work

New times of minima of some eclipsing binary stars

Year: 2017

Type: article

Abstract: Detector:Apogee ALTA U47 CCD camera, Peltier cooling, E2V CCD47-10 chip, 15 ′ × 15 ′ FOV, 1024 × 1024 pixels.Apogee ALTA U42 CCD camera, Peltier cooling, E2V CCD47-10 chip, 15 ′ × 15 ′ FOV, 2048 × 2048 pixels.ST237 camera, Peltier cooling, TC237 chip, 11 ′ × 8 ′ FOV, 640 × 480 pixels.STL1001E camera, Peltier cooling, KAF-1001E chip, 28 ′ × 28 ′ FOV, 1024 × 1024 pixels. Method of data reduction:Reduction of the CCD frames was made with C-MUNIPACK software (http://c-munipack.sourceforge.net/). Method of minimum determination:The minima times were computed with the Kwee -van Woerden method (Kwee & van Woerden, 1956).

Source: Information Bulletin on Variable Stars

DOI: 10.22444/ibvs.6191

Authors: I. Bulut, A. Kabas, C. Nehir, S. Allak, K. Neslihan, E. Yilan, M. Dogan, M. Günes, A. Bulut, O. Demircan

Institution: Çanakkale Onsekiz Mart Üniversitesi

Language: English

Topic: Stellar, planetary, and galactic studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: diamond

OpenAlex ID: W3021733659

FWCI:

Cites:

Cited by: 6

Related to: 10