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Fast Radio Transients: From Pulsars to Fast Radio Bursts

Invited talk

Published online by Cambridge University Press:  29 August 2019

B. W. Stappers ,
M. Caleb  and
L. N. Driessen
B. W. Stappers
Affiliation:
Jodrell Bank Centre for Astrophysics, University of Manchester, UK email: [email protected]
M. Caleb
Affiliation:
Jodrell Bank Centre for Astrophysics, University of Manchester, UK email: [email protected]
L. N. Driessen
Affiliation:
Jodrell Bank Centre for Astrophysics, University of Manchester, UK email: [email protected]
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Abstract

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The radio sky is full of transients, their time-scales ranging from nanoseconds to decades. Recent developments in technology sensitivity and computing capabilities have opened up the short end of that range, and are revealing a plethora of new phenomenologies. Studies of radio transients were previously restricted to analyses of archived data, but are now including real-time analyses. We focus here on Fast Radio Bursts, discuss and compare the properties of the population, and describe what is to date the only known repeating Fast Radio Burst and its host galaxy. We also review what will be possible with the new instrumentation coming online.

Keywords

Stars: neutronblack hole physicstelescopes
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S339: Southern Horizons in Time-Domain Astronomy , November 2017 , pp. 27 - 32
Copyright
© International Astronomical Union 2019 

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