Original paper can be found at: http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomical Society of the PacificUsing ROSAT observations, we estimate gas pressures in the X-ray-emitting media surrounding 63 FR II radio galaxies and quasars. We compare these pressures with the internal pressures of the radio-emitting plasma estimated by assuming minimum energy or equipartition. The majority of the radio sources (including 12/13 sources with modelled, spatially resolved X-ray emission) appear to be underpressured with respect to the external medium, suggesting that simple minimum-energy arguments underestimate the sources' internal energy densities. Some consequences of this result are discussed
We present the results of new XMM observations of FR-I and FR-II radio galaxies that show the import...
We study the radio power of the core and its relation to the optical properties of the host galaxy i...
A sample of powerful classical double radio sources, also known as FR II sources, has been assembled...
The definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI...
Discussed here are simple methods by which the densities and pressures of the gas confining double r...
The properties of very powerful extended (FR II) radio sources can be used to probe their gaseous en...
Original paper can be found at: http://www.aoc.nrao.edu/events/xraydio/We present the results of new...
We present a detailed study of the environments of a sample of nine low-power [Fanaroff–Riley type I...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASPThe intera...
‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing D...
Several models developed to describe the properties of FRIIa and FRIIb radio sources are compared an...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical...
FRIIb radio sources axe a special subset of all classical double radio sources with particularly sim...
We present results of a numerical integration of the hydrodynamical equations governing the self-sim...
We present the results of new XMM observations of FR-I and FR-II radio galaxies that show the import...
We study the radio power of the core and its relation to the optical properties of the host galaxy i...
A sample of powerful classical double radio sources, also known as FR II sources, has been assembled...
The definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI...
Discussed here are simple methods by which the densities and pressures of the gas confining double r...
The properties of very powerful extended (FR II) radio sources can be used to probe their gaseous en...
Original paper can be found at: http://www.aoc.nrao.edu/events/xraydio/We present the results of new...
We present a detailed study of the environments of a sample of nine low-power [Fanaroff–Riley type I...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASPThe intera...
‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing D...
Several models developed to describe the properties of FRIIa and FRIIb radio sources are compared an...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical...
FRIIb radio sources axe a special subset of all classical double radio sources with particularly sim...
We present results of a numerical integration of the hydrodynamical equations governing the self-sim...
We present the results of new XMM observations of FR-I and FR-II radio galaxies that show the import...
We study the radio power of the core and its relation to the optical properties of the host galaxy i...
A sample of powerful classical double radio sources, also known as FR II sources, has been assembled...