activity
20062008
most citedCold molecular gas in the Perseus cluster core - Association with X-ray cavity, Halpha filaments and cooling flow -

214 citations · 439 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph200829 cited

The inverse-Compton X-ray-emitting lobes of the high-redshift giant radio galaxy 6C 0905+39

M. C. Erlund, A. C. Fabian, Katherine M. Blundell

We present new XMM-Newton data of the high-redshift (z=1.883), Mpc-sized giant radio galaxy 6C 0905+39. The larger collecting area and longer observation time for our new data mean…

astro-ph20087 cited

The Compton-thick quasar at the heart of the high-redshift giant radio galaxy 6C 0905+39

M. C. Erlund, A. C. Fabian, Katherine M. Blundell +1

Our XMM-Newton spectrum of the giant, high-redshift (z=1.88) radio galaxy 6C 0905+39 shows that it contains one of the most powerful, high-redshift, Compton-thick quasars known. It…

astro-ph200716 cited

The luminous X-ray hotspot in 4C 74.26: synchrotron or inverse-Compton emission?

M. C. Erlund, A. C. Fabian, Katherine M. Blundell +2

We report the discovery of an X-ray counterpart to the southern radio hotspot of the largest-known radio quasar 4C 74.26 (whose redshift is z=0.104). Both XMM-Newton and Chandra im…

astro-ph2006116 cited

Radiative pressure feedback by a quasar in a galactic bulge

A. C. Fabian, A. Celotti, M. C. Erlund

We show that Eddington-limited black hole luminosities can be sufficient to deplete a galaxy bulge of gas through radiation pressure, when the ionization state of the gas and the p…

astro-ph200657 cited

Extended inverse-Compton emission from distant, powerful radio galaxies

M. C. Erlund, A. C. Fabian, Katherine M. Blundell +2

We present Chandra observations of two relatively high redshift FRII radio galaxies, 3C 432 and 3C 191 (z=1.785 and z=1.956 respectively), both of which show extended X-ray emissio…

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…