Studies on slow radio transients
Creators
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1.
National Radio Astronomy Observatory
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2.
California Institute of Technology
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3.
National Centre for Radio Astrophysics
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4.
University of Warsaw
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5.
Jagiellonian University
Abstract
We present a brief overview of a very extensive study of the group of active galactic nuclei (AGNs) that transitioned to the radio-loud state over the past few decades. The sample consists of 12 sources, both quasars and galaxies, showing the characteristics of the gigahertz-peaked spectrum objects undergoing relatively rapid changes, due to the evolution of their newly born radio jets. Discussed objects also show a wide range of physical parameters such as bolometric luminosity, black hole mass, and jet power, suggesting a great diversity among young AGNs and their hosts. Furthermore, we introduce a new observational project, the aim of which will be to investigate and gain a more in-depth understanding of the phenomenon of slow radio transients.
Additional Information
© 2021 Wiley-VCH GmbH. Issue Online: 28 December 2021; Version of Record online: 22 November 2021; Manuscript accepted: 12 October 2021; Manuscript received: 12 October 2021. MKB and AW acknowledge support from the National Science Centre, Poland under grant no. 2017/26/E/ST9/00216.Attached Files
Accepted Version - 2201.01175.pdf
Files
2201.01175.pdf
Files
(2.7 MB)
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Additional details
Identifiers
- Eprint ID
- 112086
- Resolver ID
- CaltechAUTHORS:20211130-162355557
Related works
- Describes
- https://arxiv.org/abs/2201.01175 (URL)
Funding
- National Science Centre (Poland)
- 2017/26/E/ST9/00216
Dates
- Created
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2021-11-30Created from EPrint's datestamp field
- Updated
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2022-01-28Created from EPrint's last_modified field