The evolution of a pre-heated intergalactic medium
Open Access
- 1 January 2009
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society: Letters
- Vol. 392 (1) , L26-L30
- https://doi.org/10.1111/j.1745-3933.2008.00577.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 28 references indexed in Scilit:
- Possible evidence for an inverted temperature–density relation in the intergalactic medium from the flux distribution of the Lyα forestMonthly Notices of the Royal Astronomical Society, 2008
- The Chemical Enrichment of the ICM from Hydrodynamical SimulationsSpace Science Reviews, 2008
- An improved measurement of the flux distribution of the Ly forest in QSO absorption spectra: the effect of continuum fitting, metal contamination and noise propertiesMonthly Notices of the Royal Astronomical Society, 2007
- A Census of Baryons in Galaxy Clusters and GroupsThe Astrophysical Journal, 2007
- Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numericsMonthly Notices of the Royal Astronomical Society, 2006
- Entropy amplification from energy feedback in simulated galaxy groups and clustersMonthly Notices of the Royal Astronomical Society, 2005
- The Lyman a forest opacity and the metagalactic hydrogen ionization rate at z 2-4Monthly Notices of the Royal Astronomical Society, 2005
- Revisiting the cosmic cooling crisisMonthly Notices of the Royal Astronomical Society, 2001
- Effects of Preheating on X‐Ray Scaling Relations in Galaxy ClustersThe Astrophysical Journal, 2001
- Parameter tests within cosmological simulations of galaxy formationMonthly Notices of the Royal Astronomical Society, 2000