‘The definitive version is available at www3.interscience.wiley.com '. Copyright Blackwell Publishing / Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2008.13959.xPeer reviewe
none8siWe present an analysis of deep Chandra X-ray observations of the galaxy cluster MS 0735.6+742...
When galaxy clusters collide, they generate shock fronts in the hot intracluster medium. Observation...
We present results from a 42 ks Chandra/ACIS-S observation of the transitional FR I/FR II radio gala...
Original article can be found at: http://www.journals.uchicago.edu/ApJ/--Copyright American Astronom...
Shock heating by radio jets is potentially an important process in a range of environments, as it wi...
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio g...
Extended, steep, and ultra-steep spectrum radio emission in a galaxy cluster is usually associated w...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We analysed a deep Chandra observation (334 ks) of the galaxy cluster Abell 115 and detected a shock...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
The definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI...
NGC 326 is one of the most prominent "X"- or "Z"-shaped radio galaxies (XRGs/ZRGs) and has been ...
CIZA J2242.8+5301, a merging galaxy cluster at z = 0.19, hosts a double-relic system and a faint rad...
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio g...
We use a 54.4 ks Chandra observation to study nuclear outflow activity in NGC4552 (M89), an elliptic...
none8siWe present an analysis of deep Chandra X-ray observations of the galaxy cluster MS 0735.6+742...
When galaxy clusters collide, they generate shock fronts in the hot intracluster medium. Observation...
We present results from a 42 ks Chandra/ACIS-S observation of the transitional FR I/FR II radio gala...
Original article can be found at: http://www.journals.uchicago.edu/ApJ/--Copyright American Astronom...
Shock heating by radio jets is potentially an important process in a range of environments, as it wi...
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio g...
Extended, steep, and ultra-steep spectrum radio emission in a galaxy cluster is usually associated w...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We analysed a deep Chandra observation (334 ks) of the galaxy cluster Abell 115 and detected a shock...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
The definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI...
NGC 326 is one of the most prominent "X"- or "Z"-shaped radio galaxies (XRGs/ZRGs) and has been ...
CIZA J2242.8+5301, a merging galaxy cluster at z = 0.19, hosts a double-relic system and a faint rad...
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio g...
We use a 54.4 ks Chandra observation to study nuclear outflow activity in NGC4552 (M89), an elliptic...
none8siWe present an analysis of deep Chandra X-ray observations of the galaxy cluster MS 0735.6+742...
When galaxy clusters collide, they generate shock fronts in the hot intracluster medium. Observation...
We present results from a 42 ks Chandra/ACIS-S observation of the transitional FR I/FR II radio gala...
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