An Analysis of BeppoSAX LECS Observations of EUV Emission in Clusters of Galaxies
arXiv:astro-ph/0112337 · doi:10.1086/339136
Abstract
Kaastra et al. (1999) have used the BeppoSAX LECS instrument to search for excess EUV emission in Abell 2199. They claim that the results obtained confirm an independent report of an excess EUV emission in this cluster (Lieu et al. 1999). Using an inflight derived procedure that is better suited to the analysis of extended sources and which avoids uncertainties related to ground-based calibrations for the overall detector sensitivity profile, we find no excess EUV emission in Abell 2199. We also used these procedures to search for an EUV excess in Abell 1795, but no excess was found.
6 pages, 4 figures, accepted for publication in ApJ Letters
References in corpus (3)
Cited by in corpus (12)
- The Search for the Missing Baryons at Low Redshift
- EGRET upper limits on the high-energy gamma-ray emission of galaxy clusters
- Nonthermal Particles and Radiation Produced by Cluster Merger Shocks
- Soft X-ray excess emission in clusters of galaxies observed with XMM-Newton
- On the non-thermal high energy radiation of galaxy clusters
- Soft X-ray and extreme ultraviolet excess emission from clusters of galaxies
- On the Lack of a Soft X-Ray Excess from Clusters of Galaxies
- Simulating the Soft X-ray excess in clusters of galaxies
- A Cosmic ALP Background and the Cluster Soft X-ray Excess in A665, A2199 and A2255
- Low-energy X-ray emission from the Abell 2199 cluster of galaxies
- Uniformity of foreground Galactic neutral Hydrogen over cooling flow clusters
- EUV excess in the inner Virgo cluster