Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
about
Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift.Modelling interstellar physics and chemistry: implications for surface and solid-state processes.Kinematics and excitation of the molecular hydrogen accretion disc in NGC 1275Models of AGN feedbackCold gas dynamics in Hydra-A: evidence for a rotating discHerschel observations of extended atomic gas in the core of the Perseus clusterA very extended molecular web around NGC 1275
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Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
description
article publié dans la revue scientifique Astronomy and Astrophysics
@fr
im April 2008 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in Astronomy and Astrophysics
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована у квітні 2008
@uk
name
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
@en
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
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type
label
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
@en
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
@nl
prefLabel
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
@en
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
@nl
P2093
P2860
P1476
Cold gas in the Perseus cluster core: excitation of molecular gas in filaments
@en
P2093
A. C. Edge
N. A. Hatch
R. M. Johnstone
P2860
P304
P356
10.1051/0004-6361:200809493
P407
P577
2008-04-16T00:00:00Z
P818
P819
2008A&A...484..317S