%0 Journal Article
%A Gomes, J. M.
%A Papaderos, P.
%A Vílchez, J. M.
%A Kehrig, C.
%A Iglesias Páramo, J.
%A Breda, I.
%A Lehnert, M. D.
%A Sánchez, S. F.
%A Ziegler, B.
%A dos Reis, S. N.
%A Bland Hawthorn, J.
%A Galbany, L.
%A Bomans, D. J.
%A Rosales Ortega, F. F.
%A Walcher, C. J.
%A García Benito, R.
%A Márquez, I.
%A del Olmo, A.
%A Mollá, M.
%A Marino, Raffaella Anna
%A Catalán Torrecilla, Cristina
%A González Delgado, R. M.
%A López Sánchez, Á. R.
%A CALIFA Team
%T Spiral-like star-forming patterns in CALIFA early-type galaxies
%D 2016
%@ 1432-0746
%U https://hdl.handle.net/20.500.14352/24443
%X Based on a combined analysis of SDSS imaging and CALIFA integral field spectroscopy data, we report on the detection of faint (24 <μr mag/□″< 26) star-forming spiral-arm-like features in the periphery of three nearby early-type galaxies (ETGs). These features are of considerable interest because they document the still ongoing inside-out growth of some local ETGs and may add valuable observational insight into the origin and evolution of spiral structure in triaxial stellar systems. A characteristic property of the nebular component in the studied ETGs, classified i+, is a two-radial-zone structure, with the inner zone that displays faint (EW(Hα) ≃ 1 Å) low-ionization nuclear emission-line region (LINER) properties, and the outer one (3 Å <EW(Hα)≲ 20 Å) Hii-region characteristics. This spatial segregation of nebular emission in two physically distinct concentric zones calls for an examination of aperture effects in studies of type i+ ETGs with single-fiber spectroscopic data.
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