110 citations · 158 across the 4 of their papers we have counts for
11 papers
H-X-ray Surface Brightness Correlation for Filaments in Cooling Flow Clusters
Valeria Olivares, Adrien Picquenot, Yuanyuan Su +4
Massive galaxies in cooling flow clusters display clear evidence of feedback from Active Galactic Nuclei (AGN). Joint X-ray and radio observations have shown that AGN radio jets pu…
Excitation mechanisms in the intracluster filaments surrounding Brightest Cluster Galaxies
F. L. Polles, P. Salomé, P. Guillard +12
The excitation of the filamentary gas structures surrounding giant elliptical galaxies at the center of cool-core clusters, a.k.a BCGs (brightest cluster galaxies), is key to our u…
Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
S. C. Madden, D. Cormier, S. Hony +11
While the CO(1-0) transition is often used to deduce the total molecular hydrogen in galaxies, it is challenging to detect in low metallicity galaxies, in spite of the star formati…
DeGaS-MC: Dense Gas Survey in the Magellanic Clouds I -- An APEX survey of HCO+ and HCN(2-1) toward the LMC and SMC
M. Galametz, A. Schruba, C. De Breuck +9
Investigating star formation requires precise knowledge of the properties of the dense molecular gas. The low metallicity and wide range of star formation activity of the Large and…
The CO-dark molecular gas mass in 30 Doradus
Mélanie Chevance, Suzanne C. Madden, Christian Fischer +16
Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular gas mass. However, despite bein…
Physical conditions in the gas phases of the giant HII region LMC-N11: II. Origin of [CII] and fraction of CO-dark gas
V. Lebouteiller, D. Cormier, S. C. Madden +11
(abridged) The ambiguous origin of [CII] 158um in the interstellar medium complicates its use for diagnostics concerning the star-formation rate and physical conditions in photodis…