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Parkes observations for project P1011 semester 2019APRS_13

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Parkes observations for project P1011 semester 2019APRS_13


Pulsars with features in their radio spectra, such as curvature or breaks seem to be special cases among the known pulsar population, with only about 20 per cent exhibiting them. Unfortunately, reliable flux density measurements besides at 1.4 GHz are often unavailable, so that their spectral morphologies and features cannot be determined accuratel... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5d159f9d027b7


01 Apr 2019


30 Sep 2019


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pulsars neutron stars P1011_2019APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Jankowski, Fabian; Stappers, Benjamin; Keane, Evan (2019): Parkes observations for project P1011 semester 2019APRS_13. v1. CSIRO. Data Collection. https://doi.org/10.25919/5d159f9d027b7


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/P1011-2019APRS_13


About this Project

Australia Telescope National Facility


P1011 - A wideband survey of pulsars with spectral features


Pulsars are rapidly rotating and heavily magnetized neutron stars, city-sized objects that have masses that are greater than that of our Sun. They are visible through their radio emission in the form of pulses that reach the observatory when the beam sweeps past our line of sight. However, the physical processes that make pulsars shine at radio fre... more


Observation


Parkes


Fabian Jankowski


Benjamin Stappers


Evan Keane


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