In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2
B. Debski
Details:
Year, pages: 2019, 258 - 263
Language: eng
Keywords:
stars, contact binaries, starspots
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2019/Vol_49/No_2/pp258-263_abstract.html
About article:
A new effect concerning the light curves of contact binaries is presented. The separation between the brightness maxima tends to be larger than half of the orbital phase, if the primary minimum is defined as during which the more massive star is being eclipsed.
How to cite:
ISO 690:
Debski, B. 2019. A relation between the brightness maxima separation and mass ratio in contact binaries. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no.2, pp. 258-263. 1335-1842.
APA:
Debski, B. (2019). A relation between the brightness maxima separation and mass ratio in contact binaries. Contributions of the Astronomical Observatory Skalnaté Pleso, 49(2), 258-263. 1335-1842.
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 5. 2019
Rights: