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Parkes observations for project P1032 semester 2019OCTS_04

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Parkes observations for project P1032 semester 2019OCTS_04


We propose timing observations of southern double neutron star (DNS) systems to obtain precise estimates of the component masses and thus increase the statistics of neutron star mass distribution. The improved sensitivity of the Ultra Wideband Low (UWL) receiver will provide a 3X increase in the precision of the time of arrivals (ToAs) of the pu... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5dc72d61a4593


01 Oct 2019


31 Mar 2020


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pulsars neutron stars P1032_2019OCTS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Venkatraman Krishnan, Vivek; Kramer, Michael; Freire, Paulo; Champion, David; Buchner, Sarah; Parthasarathy, Aditya; Lower, Marcus (2019): Parkes observations for project P1032 semester 2019OCTS_04. v1. CSIRO. Data Collection. https://doi.org/10.25919/5dc72d61a4593


All Rights (including copyright) CSIRO 2019.


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

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More about this Collection

ivo://au.csiro.atnf/P1032-2019OCTS_04


About this Project

Australia Telescope National Facility


P1032 - Mass measurements of southern binary pulsar systems


Even after 50 years since the discovery of neutron stars as radio pulsars, their internal composition has remained elusive. Several models have been proposed for the internal structure of neutron stars, each defining a maximum mass that neutron stars can possess. Searching for and finding very heavy neutron stars have the ability to rule out models... more


Observation


Parkes


Vivek Venkatraman Krishnan


Michael Kramer


Paulo Freire


David Champion


Sarah Buchner


Aditya Parthasarathy


Marcus Lower


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