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

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

We present a multiwavelength morphological analysis of star-forming clouds and filaments in the central (≲50 kpc) regions of 16 low-redshift (z < 0.3) cool core brightest cluster galaxies. New Hubble Space Telescope imaging of far-ultraviolet continuum emission from young (≲10 Myr), massive (≳5 M...

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Main Authors: Tremblay, G. R. (Author), O'Dea, C. P. (Author), Baum, S. A. (Author), Mittal, R. (Author), Combes, F. (Author), Li, Y. (Author), McNamara, B. R. (Author), Bremer, M. N. (Author), Clarke, T. E. (Author), Donahue, M. (Author), Edge, A. C. (Author), Fabian, A. C. (Author), Hamer, S. L. (Author), Hogan, M. T. (Author), Oonk, J. B. R. (Author), Quillen, A. C. (Author), Sanders, J. S. (Author), Salomé, P. (Author), Voit, G. M. (Author), McDonald, Michael A. (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Oxford University Press, 2017-04-21T13:43:19Z.
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