Now showing items 1-2 of 2

    • Catalán Torrecilla, C.; Gil de Paz, A.; Castillo Morales, A.; Iglesias Páramo, J.; Sánchez, S. F.; Kennicutt, R. C.; Pérez González, P. G.; Marino, R. A.; Walcher, C. J.; Husemann, B.; García Benito, R.; Mast, D.; González Delgado, R. M.; Muñoz Mateos, J. C.; Bland Hawthorn, J.; Bomans, D. J.; Olmo, A. del; Galbany, Lluis; Gomes, J. M.; Kehrig, C.; López Sánchez, Ángel R.; Mendoza, M. A.; Monreal Ibero, A.; Pérez Torres, M.; Sánchez Blázquez, P.; Vilchez, J. M. (ESO, 2015)
      Context. The star formation rate (SFR) is one of the main parameters used to analyze the evolution of galaxies through time. The need for recovering the light reprocessed by dust commonly requires the use of low spatial ...
    • Querejeta, M.; Schinnerer, E.; Meidt, S.; Sun, J.; Leroy, A. K.; Emsellem, E.; Klessen, R. S.; Muñoz Mateos, J. C.; Salo, H.; Laurikainen, E.; Beslic, I.; Blanc Mendiberri, Guillermo Alberto; Chevance, M.; Dale, D. A.; Eibensteiner, C.; Faesi, C.; García Rodríguez, A.; Glover, S. C. O.; Grasha, K.; Henshaw, J.; Herrera, C.; Hughes, A.; Kreckel, K.; Kruijssen, J. M. D.; Liu, D.; Murphy, E. J.; Pan, H-A; Pety, J.; Razza, Alessandro; Rosolowsky, E.; Saito, T.; Schruba, A.; Usero, A.; Watkins, E. J.; Williams, T. G. (EDP, 2021)
      We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct morphological masks of sub-galactic environments based on Spitzer 3.6 mu m images. At the simplest level, we distinguish five environments: ...