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Parkes observations for project P976 semester 2018APRS_13

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Parkes observations for project P976 semester 2018APRS_13


Spider pulsars - black widows (BW) and redbacks (RB) - reside in incredibly tight orbits with low-mass stellar companions. The close proximity of the two orbiting bodies leads to heavy irradiation of the companion by the pulsar wind, causing material to be driven from its surface. This excess material is not gravitationally bound to the star, and t... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5d15916a7af46


01 Apr 2018


31 Mar 2021


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pulsars neutron stars magnetic fields P976_2018APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Polzin, Elliott; Johnston, Simon; Roberts, Mallory; Oslowski, Stefan; Sobey, Charlotte; Breton, Rene (2018): Parkes observations for project P976 semester 2018APRS_13. v1. CSIRO. Data Collection. https://doi.org/10.25919/5d15916a7af46


All Rights (including copyright) CSIRO 2018.


Access to this collection's metadata and/or files (if any) are restricted until 30 Mar 2020.

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More about this Collection

ivo://au.csiro.atnf/P976-2018APRS_13


About this Project

Australia Telescope National Facility


P976 - Wide-band characterisation of the radio eclipses of black widows and redbacks


Millisecond pulsars are remnants of supernova explosions that, despite being only 20 km in diameter, are more massive than the Sun. Their name arises from the fact that they spin so fast as to complete a rotation once every few milliseconds. Beams of radio waves are emitted from their magnetic poles, which we can detect on Earth as a pulse as the b... more


Observation


Parkes


Elliott Polzin


Simon Johnston


Mallory Roberts


Stefan Oslowski


Charlotte Sobey


Rene Breton


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