Browsing by Author "66dd5a07-cf6c-4bbe-a931-b1520589ac58"

Now showing items 1-3 of 3

    • Nearby supernova host galaxies from the CALIFA survey II. Supernova environmental metallicity 
      Galbany, Lluis; Stanishev, Vallery; Mourão, A. M.; Rodrigues, M.; Flores, H.; Walcher, C. J.; Sánchez, S. F.; García Benito, R.; Mast, D.; Badenes, Carles; González Delgado, R. M.; Kehrig, C.; Lyubenova, Mariyana; Marino, R. A.; Mollá, M.; Meidt, Sharon; Pérez, E.; van de Ven, G.; Vílchez, J. M. (EDP Sciences, 2016)
      The metallicity of a supernova progenitor, together with its mass, is one of the main parameters that can rule the progenitor's fate. We present the second study of nearby supernova (SN) host galaxies (0.005 < z < 0.03) ...
    • Star formation along the Hubble sequence Radial structure of the star formation of CALIFA galaxies 
      González Delgado, R. M.; Cid Fernandes, R.; Pérez, E.; García Benito, R.; López Fernández, R.; Lacerda, E. A. D.; Cortijo Ferrero, C.; de Amorim, A. L.; Vale Asari, N.; Sánchez, S. F.; Walcher, C. J.; Wisotzki, Lutz; Mast, D.; Alves, J.; Ascasibar, Y.; Bland Hawthorn, J.; Galbany, Lluis; Kennicutt, R. C.; Márquez, I.; Masegosa Ataz, Jose; Mollá, M.; Sánchez Blázquez, P.; Vílchez, J. M. (EDP Sciences, 2016)
      The spatially resolved stellar population content of today's galaxies holds important information for understanding the different processes that contribute to the star formation and mass assembly histories of galaxies. The ...
    • Warm ionized gas in CALIFA early-type galaxies 2D emission-line patterns and kinematics for 32 galaxies 
      Gomes, J.M.; Papaderos, P.; Kehrig, C.; Vílchez, J. M.; Lehnert, M. D.; Sánchez, S. F.; Ziegler, B.; Breda, I.; dos Reis, S.N.; Iglesias-Páramo, J.; Bland-Hawthorn, J.; Galbany, Lluis; Bomans, D. J.; Rosales-Ortega, F. F.; Cid Fernandes, R.; Walcher, C. J.; Falcón Barroso, J.; García-Benito, R.; Márquez, I.; Olmo, A. del; Masegosa, J.; Mollá, M.; Marino, R. A.; González Delgado, R. M.; López Sánchez, Ángel R. (ESO, 2016-04)
      Context. The morphological, spectroscopic, and kinematical properties of the warm interstellar medium (wim) in early-type galaxies (ETGs) hold key observational constraints to nuclear activity and the buildup history of ...