Journal article
DIFFUSE CLUSTER-LIKE RADIO EMISSION IN POOR ENVIRONMENTS
The Astronomical journal, Vol.137(2), pp.3158-3171
02/01/2009
DOI: 10.1088/0004-6256/137/2/3158
Abstract
We present a study of the spectral, polarimetric, morphological, and environmental properties of the diffuse radio source 0809+39 using observations taken with the Westerbork Synthesis Radio Telescope, the Very Large Array, and archival optical and X-ray data. The source has two distinct diffuse, steep-spectrum components, one in the north that is highly polarized, and a linear southern component undetected in polarization. We discuss several plausible origins for each component, and conclude that the northern bright polarized component is most likely a radio relic associated with a poor z similar to 0.2 cluster of galaxies, with a radio/X-ray luminosity ratio two orders of magnitude above typical values. The southern component is aligned with a more extended filament of galaxies similar to 5 Mpc long at z similar to 0.04. Deep optical and X-ray follow-ups are still needed in order to confirm and understand the physical origins of the synchrotron emission. Whatever the details of these origins, 0809+39 highlights the utility of synchrotron radiation for illuminating the diffuse components of low density environments unrelated to rich clusters.
Details
- Title: Subtitle
- DIFFUSE CLUSTER-LIKE RADIO EMISSION IN POOR ENVIRONMENTS
- Creators
- Shea Brown - University of MinnesotaLawrence Rudnick - University of Minnesota
- Resource Type
- Journal article
- Publication Details
- The Astronomical journal, Vol.137(2), pp.3158-3171
- DOI
- 10.1088/0004-6256/137/2/3158
- ISSN
- 0004-6256
- eISSN
- 1538-3881
- Publisher
- Iop Publishing Ltd
- Number of pages
- 14
- Grant note
- 0908668 / Direct For Mathematical & Physical Scien; National Science Foundation (NSF); NSF - Directorate for Mathematical & Physical Sciences (MPS)
- Language
- English
- Date published
- 02/01/2009
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984428826602771
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