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Parkes observations for project P1033 semester 2019OCTS_03

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Parkes observations for project P1033 semester 2019OCTS_03


Neutron stars are composed of the densest form of matter known to exist in our universe, and thus provide a unique laboratory for exploring supra-nuclear densities. We propose timing observations of a super-massive pulsar, PSR J1748?2021B, that resides in a binary system in the NGC6440 globular cluster. This pulsar is potentially the most massiv... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5e0cab36400ba


01 Oct 2019


31 Mar 2020


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pulsars neutron stars P1033_2019OCTS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Venkatraman Krishnan, Vivek; Freire, Paulo (2019): Parkes observations for project P1033 semester 2019OCTS_03. v1. CSIRO. Data Collection. https://doi.org/10.25919/5e0cab36400ba


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/P1033-2019OCTS_03


About this Project

Australia Telescope National Facility


P1033 - Estimating the Shapiro delay in the binary pulsar system PSR J1748-2021B


Neutron stars are composed of the densest form of matter known to exist in our universe, and thus provide a unique laboratory for exploring supra-nuclear densities. Even after 50 years since the discovery of neutron stars as radio pulsars, their internal composition has remained elusive. Finding heavy neutron stars is one of the best ways to under... more


Observation


Parkes


Vivek Venkatraman Krishnan


Paulo Freire


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