X-RAY NUCLEAR ACTIVITY IN S4G BARRED GALAXIES: NO LINK BETWEEN BAR STRENGTH AND CO-OCCURRENT SUPERMASSIVE BLACK HOLE FUELING

Mauricio Cisternas(Universidad de La Laguna), Mark Seibert(Carnegie Observatories), J. H. Knapen(University of Hertfordshire), Sharon E. Meidt(Max Planck Institute for Astronomy), Dennis Zaritsky(University of Arizona), H. Salo(University of Oulu), S. Comerón(University of Oulu), A. Gil de Paz(Universidad Complutense de Madrid), Trisha Mizusawa(Florida Institute of Technology), Bruce G. Elmegreen(IBM (United States)), A. Bosma(Centre National de la Recherche Scientifique), J. L. Hinz, S. Díaz-García(University of Oulu), Luis C. Ho(Peking University), Dimitri A. Gadotti, E. Athanassoula(Laboratoire d’Astrophysique de Marseille), Benne W. Holwerda, Karín Menéndez‐Delmestre(Universidade Federal do Rio de Janeiro), Jarkko Laine(University of Oulu), Kartik Sheth(National Radio Astronomy Observatory), O. González-Martín, Michael W. Regan(Space Telescope Science Institute), Taehyun Kim(Seoul National University), Santiago Erroz-Ferrer(Universidad de La Laguna), J. C. Muñoz-Mateos(European Southern Observatory), E. Laurikainen(University of Turku)

The Astrophysical Journal

September 25, 2013

Cited by 73

|The Astrophysical Journal|2002|2.6k

|The Astrophysical Journal|2009|1.5k

|Astronomy and Astrophysics|2011|1.3k

|The Astrophysical Journal Supplement Series|2007|519

|Astronomy and Astrophysics|2014|514

X-RAY NUCLEAR ACTIVITY IN S<sup>4</sup>G BARRED GALAXIES: NO LINK BETWEEN BAR STRENGTH AND CO-OCCURRENT SUPERMASSIVE BLACK HOLE FUELING