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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

Hamuy Wackenhut, MarioPhillips, M. M.Suntzeff, Nicholas B.Schommer, R. A.Maza Sancho, JoséAntenaza, RobertoWischnjewsky, MarinaValladares, GeraldoMuena, CésarGonzález, L. E.Avilés, R.Wells, LisaSmith, R. C.Navarrete, MauricioCovarrubias, RicardoWilliger, G.Walker, Alistair R.Layden, A. C.Elias, J. H.Baldwin, J. A.Hernández, ManuelTirado, HernánUgarte, PatricioElston, R.Saavedra, NelsonBarrientos, FelipeCosta Hechenleitner, EdgardoLira Teillery, PaulinaRuiz González, María TeresaAnguita, ClaudioGómez, XimenaOrtiz, P.Della Valle, M.Danziger, J.Storm, J.Kim, Y. C.Bailyn, C.Rubenstein, Eric P.Tucker, D.Cersosimo, S.Méndez Bussard, René AlejandroSiciliano, L.Sherry, W.Chaboyer, BrianKoopmann, R. A.Geisler, D.Sarajedini, A.Dey, ArjunTyson, N.Rich, R. MichaelGal, R.Lamontagne, RobertCaldwell, N.Guhathakurta, PuragraPhillips, A. C.Szkody, P.Prosser, C.Ho, Luis C.McMahan, R.Baggley, G.Cheng, K. P.Havlen, R.Wakamatsu, K.Janes, Kenneth A.Malkan, MathewBaganoff, F.Seitzer, P.Shara, M.Sturch, C.Hesser, J.Hartigan, P.Hughes, J.Welch, D. L.Williams, T. B.Ferguson, H.Francis, P. J.French, L.Bolte, M.Roth, J.Odewahn, S.Howell, S.Krzeminski, W.[BVRI light curves for 29 type Ia supernovae]

Hamuy Wackenhut, MarioPhillips, M. M.Suntzeff, Nicholas B.Schommer, R. A.Maza Sancho, JoséAntenaza, RobertoWischnjewsky, MarinaValladares, GeraldoMuena, CésarGonzález, L. E.Avilés, R.Wells, LisaSmith, R. C.Navarrete, MauricioCovarrubias, RicardoWilliger, G.Walker, Alistair R.Layden, A. C.Elias, J. H.Baldwin, J. A.Hernández, ManuelTirado, HernánUgarte, PatricioElston, R.Saavedra, NelsonBarrientos, FelipeCosta Hechenleitner, EdgardoLira Teillery, PaulinaRuiz González, María TeresaAnguita, ClaudioGómez, XimenaOrtiz Arce, PatricioDella Valle, MassimoDanziger, J.Storm, J.Kim, Y. C.Bailyn, C.Rubenstein, Eric P.Tucker, D.Cersosimo, S.Méndez, R. A.Siciliano, L.Sherry, W.Chaboyer, BrianKoopmann, R. A.Geisler, D.Sarajedini, A.Dey, ArjunTyson, N.Rich, R. MichaelGal, R.Lamontagne, RobertCaldwell, N.Guhathakurta, PuragraPhillips, A. C.Szkody, P.Prosser, C.Ho, Luis C.McMahan, R.Baggley, G.Cheng, K. P.Havlen, R.Wakamatsu, K.Janes, Kenneth A.Malkan, MathewBaganoff, F.Seitzer, P.Shara, M.Sturch, C.Hesser, J.Hartigan, P.Hughes, J.Welch, D. L.Williams, T. B.Ferguson, H.Francis, P. J.French, L.Bolte, M.Roth, J.Odewahn, S.Howell, S.Krzeminski, W.[BVRI light curves for 29 type Ia supernovae]

Gieren, W.Pilecki, B.Pietrzyński, G.Graczyk, D.Udalski, A.Soszyński, I.Thompson, I.B.Moroni, P.G.P.Smolec, R.Konorski, P.Górski, M.Karczmarek, P.Suchomska, K.Taormina, M.Gallenne, A.Storm, J.Bono, G.Catelan, M.Szymański, M.Kozłowski, S.Pietrukowicz, P.Wyrzykowski, Ł.Poleski, R.Skowron, J.Minniti, D.Ulaczyk, K.Mróz, P.Pawlak, M.Nardetto, N.[THE ARAUCARIA PROJECT: A STUDY OF THE CLASSICAL CEPHEID IN THE ECLIPSING BINARY SYSTEM OGLE LMC562.05.9009 IN THE LARGE MAGELLANIC CLOUD]THE ARAUCARIA PROJECT: A STUDY OF THE CLASSICAL CEPHEID IN THE ECLIPSING BINARY SYSTEM OGLE LMC562.05.9009 IN THE LARGE MAGELLANIC CLOUD

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