Parkes observations for project P1032 semester 2020APRS_07
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... morelses compared to the multibeam data. This has the potential to perform quick
measurements of masses for a number of binary systems in the next 1-2 years. We will also use MeerKAT
observations at crucial orbital phases to increase our chances of mass measurements. Increase in the number
of measured NS masses has significant implications for understanding NS internal structure and for stellar
and binary evolution physics. less
Astronomical and Space Sciences not elsewhere classified
https://doi.org/10.25919/5f63b022bdc16
01 Apr 2020
30 Sep 2020
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pulsars
;
neutron stars
;
P1032_2020APRS
Creative Commons Attribution 4.0 International Licence
CSIRO (Australia)
Venkatraman Krishnan, Vivek; Kramer, Michael; Burgay, Marta; Freire, Paulo; Bailes, Matthew; Champion, David; Buchner, Sarah; Parthasarathy, Aditya; Lower, Marcus (2020): Parkes observations for project P1032 semester 2020APRS_07. v1. CSIRO. Data Collection.
https://doi.org/10.25919/5f63b022bdc16
All Rights (including copyright) CSIRO 2020.
Access to this collection's metadata and/or files (if any) are restricted until 30 Mar 2022.