In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2
M. Ratajczak - A. Pigulski - K. Pavlovski
Detaily:
Rok, strany: 2019, 252 - 257
Jazyk: eng
Kľúčové slová:
binaries: spectroscopic, binaries: eclipsing, stars: oscillations
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2019/Vol_49/No_2/pp252-257_abstract.html
O článku:
The analysis of eclipsing binaries with massive components enables to test stellar evolution models and track selected aspects of the structure of early-type stars. Stellar pairs with B-type components may serve to find tighter constraints on the mechanisms of convective core overshooting or masses of β Cephei-type stars. We present the results of an analysis of several eclipsing binaries — N Sco, LS CMa, and δ Vel — observed by BRITE-Constellation satellites and followed by a wide range of ground-based telescopes.
Ako citovať:
ISO 690:
Ratajczak, M., Pigulski, A., Pavlovski, K. 2019. Tracking massive pairs. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no.2, pp. 252-257. 1335-1842.
APA:
Ratajczak, M., Pigulski, A., Pavlovski, K. (2019). Tracking massive pairs. Contributions of the Astronomical Observatory Skalnaté Pleso, 49(2), 252-257. 1335-1842.
O vydaní:
Vydavateľ: Astronomical Institute, Slovak Academy of Sciences
Publikované: 1. 5. 2019
Verejná licencia:
