The competition between confinement and ram pressure and its implications for galaxies in groups and clusters
Open Access
- 2 July 2012
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 424 (2) , 1179-1186
Abstract
No abstract availableKeywords
All Related Versions
This publication has 45 references indexed in Scilit:
- DETECTION OF A HOT GASEOUS HALO AROUND THE GIANT SPIRAL GALAXY NGC 1961The Astrophysical Journal, 2011
- X-ray coronae in simulations of disc galaxy formationMonthly Notices of the Royal Astronomical Society, 2010
- Galaxies intergalactic medium interaction calculation I. Galaxy formation as a function of large-scale environmentMonthly Notices of the Royal Astronomical Society, 2009
- Substructures in hydrodynamical cluster simulationsMonthly Notices of the Royal Astronomical Society, 2009
- INTRACLUSTER MEDIUM ENTROPY PROFILES FOR A CHANDRA ARCHIVAL SAMPLE OF GALAXY CLUSTERSThe Astrophysical Journal Supplement Series, 2009
- Simulating galactic outflows with kinetic supernova feedbackMonthly Notices of the Royal Astronomical Society, 2008
- The Hot Gas Content of Low‐Luminosity Early‐Type Galaxies and the Implications Regarding Supernova Heating and Active Galactic Nucleus FeedbackThe Astrophysical Journal, 2006
- Virial shocks in galactic haloes?Monthly Notices of the Royal Astronomical Society, 2003
- The Origin of Star Formation Gradients in Rich Galaxy ClustersThe Astrophysical Journal, 2000
- Ram pressure stripping of spiral galaxies in clustersMonthly Notices of the Royal Astronomical Society, 1999