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Parkes observations for project P888 semester 2015OCTS_BPSR_01

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Parkes observations for project P888 semester 2015OCTS_BPSR_01


Erratically-emitting neutron stars like Rotating Radio Transients (RRATs), represent approximately 3% (and increasing) of radio-emitting pulsars as they are found via searches of archival and current pulsar surveys. The sporadic emission from these sources makes them difficult to study and nearly all information about the properties of the objects ... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.4225/08/59cfb4908ffc6


01 Oct 2015


31 Mar 2016


CSIRO Enquiries
CSIROEnquiries@csiro.au
1300 363 400

pulsars neutron stars transients BPSR HIPSR


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Petroff, Emily; Johnston, Simon; van Straten, Willem; Keane, Evan; Caleb, Manisha (2016): Parkes observations for project P888 semester 2015OCTS_BPSR_01. v1. CSIRO. Data Collection. https://doi.org/10.4225/08/59cfb4908ffc6


All Rights (including copyright) CSIRO 2016.


The metadata and files (if any) are available to the public.

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More about this Collection

ivo://au.csiro.atnf/P888-2015OCTS_BPSR_01


About this Project

Australia Telescope National Facility


P888 - Expanding the rotating radio transient parameter space


Neutron stars are the result of stellar explosions (supernovae) which occur in massive stars once they have reached the ends of their lives. Most pulsars are detectable by their regular intervals of pulsed emission (occurring every few seconds, up to several hundred times a second!), which happens because the star is rotating and flashing a beam of... more


Observation


Parkes


Emily Petroff


Simon Johnston


Willem van Straten


Evan Keane


Manisha Caleb


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