Autor:
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.
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...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/4738
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
