- Abstract:
-
We have shown previously that a broad correlation between the peak radio luminosity and the variability time-scales, approximately L ∝ τ5, exists for variable synchrotron emitting sources and that different classes of astrophysical sources occupy different regions of luminosity and time-scale space. Based on those results, we investigate whether the most basic information available for a newly discovered radio variable or transient – their rise and/or decline rate – can be used to set initial...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Files:
-
-
(pdf, 3.2MB)
-
- Publisher copy:
- 10.1093/mnras/stx1744
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 471
- Issue:
- 4
- Pages:
- 3788–3805
- Publication date:
- 2017-07-14
- Acceptance date:
- 2017-07-08
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Pubs id:
-
pubs:735144
- URN:
-
uri:07366992-56d5-4347-9bf7-cbf906c6aa55
- UUID:
-
uuid:07366992-56d5-4347-9bf7-cbf906c6aa55
- Local pid:
- pubs:735144
- Language:
- English
- Keywords:
- Copyright holder:
- Pietka et al.
- Copyright date:
- 2017
- Notes:
- © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. This is the publisher's version of the article. The final version is available online from Oxford University Press at: https://doi.org/10.1093/mnras/stx1744
Journal article
On the use of variability time-scales as an early classifier of radio transients and variables
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