Original Paper
Radio wavelength transients: Current and emerging prospects
Article first published online: 4 MAR 2008
DOI: 10.1002/asna.200710935
Copyright © 2008 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
Additional Information
How to Cite
Lazio, J. (2008), Radio wavelength transients: Current and emerging prospects. Astron. Nachr., 329: 330–333. doi: 10.1002/asna.200710935
Publication History
- Issue published online: 4 MAR 2008
- Article first published online: 4 MAR 2008
- Manuscript Accepted: 27 NOV 2007
- Manuscript Received: 27 AUG 2007
Funded by
- 6.1 Base
- Abstract
- References
- Cited By
Keywords:
- gamma rays: bursts;
- pulsars: general;
- stars: flares;
- telescopes
Abstract
Known classes of radio wavelength transients range from the nearby stellar flares and radio pulsars to the distant Universe γ-ray burst afterglows. Hypothesized classes of radio transients include analogs of known objects, e.g., extrasolar planets emitting Jovian-like radio bursts and giant-pulse emitting pulsars in other galaxies, to the exotic, prompt emission from γ-ray bursts, evaporating black holes, and transmitters from other civilizations. A number of instruments and facilities are either under construction or in early observational stages and are slated to become available in the next few years. With a combination of wide fields of view and wavelength agility, the detection and study of radio transients will improve immensely. (© 2008 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

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