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pro vyhledávání: '"Puha, E"'
Autor:
Pribulla, T., Puha, E., Borkovits, T., Budaj, J., Garai, Z., Guenther, E., Hambalek, L., Komzik, R., Kundra, E., Szabo, Gy. M., Vanko, M.
VW~LMi is the tightest known quadruple system with 2+2 hierarchy. It consists of a W UMa-type eclipsing binary (P12 = 0.47755 days) and another detached non-eclipsing binary (P34 = 7.93 days) orbiting around a common center of mass is about P1234 = 3
Externí odkaz:
http://arxiv.org/abs/2003.08169
Autor:
Pribulla, T, Puha, E, Borkovits, T, Budaj, J, Garai, Z, Guenther, E, Hambálek, L, Komžík, R, Kundra, E, Szabó, Gy M, Vaňko, M
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 05/01/2020, Vol. 494 Issue 1, p178-189, 12p