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20032008
most citedCold molecular gas in the Perseus cluster core - Association with X-ray cavity, Halpha filaments and cooling flow -

214 citations · 473 across the 4 of their papers we have counts for

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astro-ph200877 cited

Cold gas in the Perseus cluster core: Excitation of molecular gas in filaments

P. Salomé, F. Combes, Y. Revaz +4

We have recently detected CO lines in the well-known filaments around NGC 1275, the galaxy at the centre of the Perseus cluster of galaxies. These previous observations, with the H…

astro-ph2007127 cited

Formation of cold filaments in cooling flow clusters

Y. Revaz, F. Combes, P. Salome

Emission-lines in the form of filamentary structures is common in bright clusters characterized by short cooling times. In the Perseus cluster, cold molecular gas, tightly linked t…

astro-ph200655 cited

Detection of HNC and tentative detection of CN at z=3.9

M. Guelin, P. Salome, R. Neri +8

Molecular line emission from high-redshift galaxies holds great promise for the study of galaxy formation and evolution. The weak signals can only be detected with the largest mm-w…

astro-ph2006214 cited

Cold molecular gas in the Perseus cluster core - Association with X-ray cavity, Halpha filaments and cooling flow -

P. Salome, F. Combes, A. C. Edge +7

Cold molecular gas has been recently detected in several cooling flow clusters of galaxies where huge optical nebulosities often stand. These optical filaments are tightly linked t…

astro-ph2003

Mapping the cold molecular gas in a cooling flow cluster: Abell 1795

P. Salome, F. Combes

Cold molecular gas is found in several clusters of galaxies (Edge, 2001, Salome' & Combes, 2003): single dish telescope observations in CO(1-0) and CO(2-1) emission lines have reve…

astro-ph2003

Cold molecular gas in cooling flow clusters of galaxies

P. Salome, F. Combes

The results of a CO line survey in central cluster galaxies with cooling flows are presented. Cold molecular gas is detected with the IRAM 30m telescope, through CO(1-0) and CO(2-1…