Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
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Cold, clumpy accretion onto an active supermassive black hole.HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus ClusterALMA observations of cold molecular gas filaments trailing rising radio bubbles in PKS 0745−191Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795
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Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
description
im Juni 2015 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в червні 2015
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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Far-ultraviolet morphology of ...... ore brightest cluster galaxies
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A. C. Edge
A. C. Quillen
B. R. McNamara
C. P. O'Dea
G. M. Voit
G. R. Tremblay
J. B. R. Oonk
M. A. McDonald
M. Donahue
M. N. Bremer
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10.1093/MNRAS/STV1151
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2015-06-29T00:00:00Z
P819
2015MNRAS.451.3768T