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Parkes observations for project P885 semester 2019APRS_09

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Parkes observations for project P885 semester 2019APRS_09


We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950 approximately weekly, to track their rotation, flux density, and polarisation, as we have been doing through this project. As of this week (8 Dec 2018), XTE J1810-197 is again a radio magnetar, after 10 years dormant! (We have been observing it sporadically during its low st... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5d41a03398c94


01 Apr 2019


30 Sep 2019


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pulsars neutron stars P885_2019APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Camilo, Fernando; Johnston, Simon; Sarkissian, John; Reynolds, John; Scholz, Paul (2019): Parkes observations for project P885 semester 2019APRS_09. v1. CSIRO. Data Collection. https://doi.org/10.25919/5d41a03398c94


All Rights (including copyright) CSIRO 2019.


Access to this collection's metadata and/or files (if any) are restricted until 30 Mar 2021.

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More about this Collection

ivo://au.csiro.atnf/P885-2019APRS_09


About this Project

Australia Telescope National Facility


P885 - Understanding the Remarkable Behaviour of Radio Magnetars


Neutron stars are extreme objects, the size of a city but containing the mass of the Sun. Pulsars are neutron stars with very strong magnetic fields that rotate rapidly and emit focused beams of radio waves that we may detect on Earth once with every turn of the star, in light-house-like fashion. While the typical pulsar has a magnetic field ... more


Observation


Parkes


Fernando Camilo


Simon Johnston


John Sarkissian


John Reynolds


Paul Scholz


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