20 citations · 22 across the 3 of their papers we have counts for
7 papers
Morphology of flows and buoyant bubbles in the Virgo cluster
Georgi Pavlovski, Christian R. Kaiser, Edward C. D. Pope +1
There is growing evidence that the active galactic nuclei (AGN) associated with the central elliptical galaxy in clusters of galaxies are playing an important role in the evolution…
Dynamics of buoyant bubbles in clusters of galaxies
Georgi Pavlovski, Christian R. Kaiser, Edward C. D. Pope
We present a phenomenological model of the dynamics of buoyant bubbles in the atmosphere of a cluster of galaxies. The derived equations describe velocity, size, mass, temperature…
Heating rate profiles in clusters of galaxies
Edward Pope, Christian Kaiser, Georgi Pavlovski +1
The results of hydrodynamic simulations of the Virgo and Perseus clusters suggest that thermal conduction is not responsible for the observed temperature and density profiles. As a…
Heating Rate Profiles in Galaxy Clusters
Edward C. D. Pope, Georgi Pavlovski, Christian R. Kaiser +1
In recent years evidence has accumulated suggesting that the gas in galaxy clusters is heated by non-gravitational processes. Here we calculate the heating rates required to mainta…
The Effect of Thermal Conduction on the Virgo Cluster
Edward C. D. Pope, Georgi Pavlovski, Christian R. Kaiser +1
Thermal conduction has been suggested as a possible mechanism by which sufficient energy is supplied to the central regions of galaxy clusters to balance the effect of radiative co…
Hydrodynamical simulations of the decay of high-speed molecular turbulence. II. Divergence from isothermality
G. Pavlovski, M. D. Smith, M. -M. Mac Low
A roughly constant temperature over a wide range of densities is maintained in molecular clouds through radiative heating and cooling. An isothermal equation of state is therefore…