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Parkes observations for project P1041 semester 2020APRS_01

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Parkes observations for project P1041 semester 2020APRS_01


We recently discovered five millisecond pulsars (MSPs) in the globular cluster Omega Centauri. This is the first pulsar discovery in this globular cluster. Four of these pulsars are isolated with spin periods of 4.1, 4.2, 4.6 and 6.8ms. The fifth has a spin period of 4.8ms and is in an eclipsing binary system with an orbital period of 2.1 hours. We... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5e96b3ea3ee98


01 Apr 2020


30 Sep 2020


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pulsars neutron stars P1041_2020APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Dai, Shi; Possenti, Andrea; Johnston, Simon; Camilo, Fernando; Kerr, Matthew; Kumamoto, Hiroki (2020): Parkes observations for project P1041 semester 2020APRS_01. v1. CSIRO. Data Collection. https://doi.org/10.25919/5e96b3ea3ee98


All Rights (including copyright) CSIRO 2020.


Access to this collection's metadata and/or files (if any) are restricted until 30 Mar 2022.

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More about this Collection

ivo://au.csiro.atnf/P1041-2020APRS_01


About this Project

Australia Telescope National Facility


P1041 - Timing of millisecond pulsars in Globular Cluster Omega Centauri


Omega Centauri is a globular cluster in the constellation of Centaurus that was first identified by Edmond Halley in 1677. Located at a distance of 15,800 light-years, it is the largest globular cluster in the Milky Way at a diameter of roughly 150 light-years. It is estimated to contain approximately 10 million stars and a total mass equivalent to... more


Observation


Parkes


Shi Dai


Andrea Possenti


Simon Johnston


Fernando Camilo


Matthew Kerr


Hiroki Kumamoto


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