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Context. The ratio of the first overtone (1O)/fundamental (F) periods of mixed-mode Cepheids that pulsate simultaneously in these two modes (F/1O) is metallicity-dependent. It can therefore be used to characterize the systems that host such variable stars. Aims. We want to take advantage of the F...


Lemasle, B.Hajdu, G.Kovtyukh, V.Inno, L.Grebel, E.K.Catelan, M.Bono, G.François, P.Kniazev, A.Da Silva, R.Storm, J.[Milky Way metallicity gradient from Gaia DR2 F/1O double-mode Cepheids]Milky Way metallicity gradient from Gaia DR2 F/1O double-mode Cepheids

Väisänen, P.Mattila, S.Kniazev, A.Adamo, A.Efstathiou, A.Farrah, D.Ohansson, P. H.Östlin, G.Buckley, D. A. H.Burgh, E. B.Crause, L.Hashimoto, Y.Lira Teillery, PaulinaLoaring, N.Nordsieck, K.Romero Colmenero, EncarniRyder, S.Still, M.Zijlstra, A.[Adaptive optics imaging and optical spectroscopy of a multiple merger in a luminous infrared galaxy]

Kniazev, A.Minniti, D. (Dante), 1962-[CHARACTERIZATION OF THE NEARBY L/T BINARY BROWN DWARF WISE J104915.57-531906.1 AT 2 pc FROM THE SUN]CHARACTERIZATION OF THE NEARBY L/T BINARY BROWN DWARF WISE J104915.57-531906.1 AT 2 pc FROM THE SUN

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