UNVEILING THE STRUCTURE OF BARRED GALAXIES AT 3.6 μm WITH THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G). I. DISK BREAKS

Taehyun Kim(Seoul National University), Trisha Mizusawa(Florida Institute of Technology), J. H. Knapen(University of Hertfordshire), Dennis Zaritsky(University of Arizona), H. Salo(University of Oulu), Barry F. Madore(California Institute of Technology), S. Comerón(University of Oulu), A. Gil de Paz(Universidad Complutense de Madrid), Mauricio Cisternas(Universidad de La Laguna), Bonita de Swardt(South African Radio Astronomy Observatory), Bruce G. Elmegreen(IBM (United States)), A. Bosma(Centre National de la Recherche Scientifique), J. L. Hinz, Luis C. Ho(Peking University), Dimitri A. Gadotti, E. Athanassoula(Laboratoire d’Astrophysique de Marseille), Myung Gyoon Lee(Seoul National University), Benne W. Holwerda, Karín Menéndez‐Delmestre(Universidade Federal do Rio de Janeiro), Jarkko Laine(University of Oulu), Kartik Sheth(National Radio Astronomy Observatory), R. Buta(University of Alabama), Michael W. Regan(Space Telescope Science Institute), Santiago Erroz-Ferrer(Universidad de La Laguna), Mark Seibert(Carnegie Observatories), Juan-Carlos Muñoz-Mateos(National Radio Astronomy Observatory), E. Laurikainen(University of Turku)

The Astrophysical Journal

January 28, 2014

Cited by 59

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UNVEILING THE STRUCTURE OF BARRED GALAXIES AT 3.6 μm WITH THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S<sup>4</sup>G). I. DISK BREAKS