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We present new theoretical period-luminosity-metallicity (PLZ) relations for RR Lyræ stars (RRLs) at Spitzer and WISE wavelengths. The PLZ relations were derived using nonlinear, time-dependent convective hydrodynamical models for a broad range of metal abundances (Z = 0.0001-0.0198). In deriving...


Neeley, J.R.Marengo, M.Bono, G.Braga, V.F.Dall'ora, M.Magurno, D.Marconi, M.Trueba, N.Tognelli, E.Moroni, P.G.P.Beaton, R.L.Freedman, W.L.Madore, B.F.Monson, A.J.Scowcroft, V.Seibert, M.Stetson, P.B.[On a New Theoretical Framework for RR Lyrae Stars. II. Mid-infrared Period-Luminosity-Metallicity Relations]On a New Theoretical Framework for RR Lyrae Stars. II. Mid-infrared Period-Luminosity-Metallicity Relations

Braga, V.F.Stetson, P.B.Bono, G.Dall'Ora, M.Ferraro, I.Fiorentino, G.Iannicola, G.Marconi, M.Marengo, M.Monson, A.J.Neeley, J.Persson, S.E.Beaton, R.L.Buonanno, R.Calamida, A.Castellani, M.Carlo, E.D.Fabrizio, M.Freedman, W.L.Inno, L.Madore, B.F.Magurno, D.Marchetti, E.Marinoni, S.Marrese, P.Matsunaga, N.Minniti, D.Monelli, M.Nonino, M.Piersimoni, A.M.Pietrinferni, A.Prada-Moroni, P.Pulone, L.Stellingwerf, R.Tognelli, E.Walker, A.R.Valenti, E.Zoccali, M.[On the RR Lyrae Stars in Globulars. V. the Complete Near-infrared (JHK s) Census of ω Centauri RR Lyrae Variables]On the RR Lyrae Stars in Globulars. V. the Complete Near-infrared (JHK s) Census of ω Centauri RR Lyrae Variables

Randich, S.Tognelli, E.Jackson, R.Jeffries, R.D.Degl'Innocenti, S.Pancino, E.Fiorentin, P.R.Spagna, A.Sacco, G.Bragaglia, A.Magrini, L.Moroni, P.G.P.Alfaro, E.Franciosini, E.Morbidelli, L.Roccatagliata, V.Bouy, H.Bravi, L.Jiménez-Esteban, F.M.Jordi, C.Zari, E.Tautvaišiene, G.Drazdauskas, A.Mikolaitis, S.Gilmore, G.Feltzing, S.Vallenari, A.Bensby, T.Koposov, S.Korn, A.Lanzafame, A.Smiljanic, R.Bayo, A.Carraro, G.Costado, M.T.Heiter, U.Hourihane, A.Jofré, P.Lewis, J.Monaco, L.Prisinzano, L.Sbordone, L.Sousa, S.G.Worley, C.C.Zaggia, S.[The Gaia -ESO Survey: Open clusters in Gaia -DR1: A way forward to stellar age calibration]The Gaia -ESO Survey: Open clusters in Gaia -DR1: A way forward to stellar age calibration

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