In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2
B. Debski
Detaily:
Rok, strany: 2019, 258 - 263
Jazyk: eng
Kľúčové slová:
stars, contact binaries, starspots
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2019/Vol_49/No_2/pp258-263_abstract.html
O článku:
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.
Ako citovať:
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.
O vydaní:
Vydavateľ: Astronomical Institute, Slovak Academy of Sciences
Publikované: 1. 5. 2019
Verejná licencia: