Measuring the non-thermal pressure in early-type galaxy atmospheres: a comparison of X-ray and optical potential profiles in M87 and NGC 1399
Open Access
- 25 July 2008
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 388 (3) , 1062-1078
- https://doi.org/10.1111/j.1365-2966.2008.13507.x
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- Cosmic Rays and Radio Halos in Galaxy Clusters: New Constraints from Radio ObservationsThe Astrophysical Journal, 2007
- Convection in Galaxy‐Cluster Plasmas Driven by Active Galactic Nuclei and Cosmic‐Ray BuoyancyThe Astrophysical Journal, 2004
- An [ITAL]XMM-Newton[/ITAL] Observation of NGC 1399 Reveals Two Phases of Hot Gas and Supersolar Abundances in the Central RegionsThe Astrophysical Journal, 2002
- An XMM-Newton study of the sub-structure in M 87's haloAstronomy & Astrophysics, 2001
- Iron Gradients in Cooling Flow Galaxies and GroupsThe Astrophysical Journal, 2000
- Stripped Spiral Galaxies as Promising Targets for the Determination of the Cepheid Distance to the Virgo ClusterThe Astrophysical Journal, 1997
- Mapping the Gas Temperature Distribution in Extended X‐Ray Sources and Spectral Analysis in the Case of Low Statistics: Application toASCAObservations of Clusters of GalaxiesThe Astrophysical Journal, 1996
- The reliability of X-ray constraints of intrinsic cluster shapesThe Astrophysical Journal, 1995
- A ROSAT HRI study of the interaction of the X-ray-emitting gas and radio lobes of NGC 1275Monthly Notices of the Royal Astronomical Society, 1993
- M/L and velocity anisotropy from observations of spherical galaxies, or must M87 have a massive black hole?Monthly Notices of the Royal Astronomical Society, 1982