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Parkes observations for project P786 semester 2012APRS

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Parkes observations for project P786 semester 2012APRS


Rotating Radio Transients (RRATs), neutron stars from which sporadic radio bursts are detected, represent approximately 3% (and increasing) of radio-emitting pulsars as they are found via single-pulse searches of archival and current pulsar surveys. Their sporadic emission makes them difficult to study and nearly all information about the propertie... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.4225/08/5338247C5CDDC


01 Apr 2012


30 Sep 2012


CSIRO Enquiries
CSIROEnquiries@csiro.au
1300 363 400

pulsars neutron stars transients


Creative Commons Attribution 3.0 Unported Licence


CSIRO (Australia)


McLaughlin, Maura; Johnston, Simon; Kramer, Michael; Lyne, Andrew; Burke-Spolaor, Sarah; Eatough, Ralph; Stappers, Benjamin; Keane, Evan; Miller, Josh; Palliyaguru, Nipuni; Young, Neil (2013): Parkes observations for project P786 semester 2012APRS. v1. CSIRO. Data Collection. https://doi.org/10.4225/08/5338247C5CDDC


All Rights (including copyright) CSIRO Australia 2013.


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

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More about this Collection

ivo://au.csiro.atnf/P786-2012APRS


About this Project

Australia Telescope National Facility


P786 - Transient Radio Neutron Stars


In 2006 a number of neutron stars were discovered by astronomers. These new sources - dubbed RRATs (eRRATic neutron stars) were seen to emit bursts of radio emission every few minutes. Neutron stars are the remnants of stellar explosions (supernovae) which occur in massive stars once they have reached the ends of their lives. The discovery of such ... more


Observation


Parkes


Maura McLaughlin


Simon Johnston


Michael Kramer


Andrew Lyne


Sarah Burke-Spolaor


Ralph Eatough


Benjamin Stappers


Evan Keane


Josh Miller


Nipuni Palliyaguru


Neil Young


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