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Parkes observations for project P995 semester 2018OCTS_20

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Parkes observations for project P995 semester 2018OCTS_20


We propose to perform observations of the very young pulsar PSR B0540–69 in the Large Magellanic Cloud to detect pulsed flux from this traditionally radio-quiet source. We are motivated to do so due to a relatively recent X-ray observation of a 36% change in its spin down rate, thought to be due to a state change in its magnetospheric proces... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5c9382ad19fbc


01 Oct 2018


01 Apr 2019


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supernovae / supernovae remnants pulsars neutron stars transients P995_2018OCTS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Ferdman, Robert; Kaspi, Victoria ; Archibald, Robert (2018): Parkes observations for project P995 semester 2018OCTS_20. v1. CSIRO. Data Collection. https://doi.org/10.25919/5c9382ad19fbc


All Rights (including copyright) CSIRO 2018.


Access to this collection's metadata and/or files (if any) are restricted until 01 Oct 2020.

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More about this Collection

ivo://au.csiro.atnf/P995-2018OCTS_20


About this Project

Australia Telescope National Facility


P995 - A search for pulsed emission from PSR~B0540–69 after a state change


PSR B0540–69 is a very young pulsar in the Large Magellanic Cloud, a satellite galaxy of our Milky Way. It was formed as a very dense, fast-spinning neutron-star remnant of a violent supernova explosion that occurred nearly 1700 years ago. We see a "pulse" with each rotation of these objects, as its emission beam sweeps past out line of sight, lik... more


Observation


Parkes


Robert Ferdman


Victoria Kaspi


Robert Archibald


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