Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies

G. Tremblay , C. O'Dea , S. Baum , R. Mittal , M. Mcdonald , F. Combes (1, 2) , Y. Li , B. Mcnamara , M. Bremer (3) , T. Clarke , M. Donahue (4) , A. Edge (5) , A. Fabian (6) , S. Hamer (1) , M. J. Hogan (7) , J. Oonk , A. Quillen , J. Sanders , P. Salomé (1) , G. Voit

1 LERMA - Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique
2 Collège de France - Chaire Galaxies et cosmologie
3 AUTRES
4 University of Michigan [Ann Arbor]
5 Department of Physics
6 Institute of Astronomy [Cambridge]
7 SLAC - SLAC National Accelerator Laboratory

Domaines: Physique [physics]; Astrophysique [astro-ph]

G. Tremblay, C. O'Dea, S. Baum, R. Mittal, M. Mcdonald, et al.. Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies. Monthly Notices of the Royal Astronomical Society, 2015, 451 (4), pp.3768-3800. ⟨10.1093/mnras/stv1151⟩. ⟨hal-02400454⟩