2019/08/31 by David Kaplan, David L. Kaplan, Shi Dai +15
Physics and Astronomy · #Astrometry #Binary pulsar #Galaxies: Formation, Evolution, Phenomena #Millisecond pulsar #Pathfinder #Point source #Proper motion #Pulsar #Pulsars and Gravitational Waves Research #Radio Astronomy Observations and Technology #Radio telescope #Telescope #astro-ph.HE
paper · pdf · doi:10.3847/1538-4357/ab397f
ApJ, in press
openalex created_date 2019/08/13 · openalex publication_date 2019/10/10 · arxiv created 2020/10/06 · arxiv updated 2020/10/08 · openalex updated_date 2026/08/05
Abstract We identified a highly polarized, steep-spectrum radio source in a deep image with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope at 888 MHz. After considering and rejecting a stellar origin for this source, we discovered a new millisecond pulsar (MSP) using observations from the Parkes radio telescope. This pulsar has period 2.77 ms and dispersion measure 228.27 pc cm −3 . Although this pulsar does not yet appear to be particularly remarkable, its short spin period, wide profile, and high dispersion measure make it relatively hard to discover through traditional blind periodicity searches. Over the course of several weeks we see changes in the barycentric period of this pulsar that are consistent with orbital motion in a binary system, but the properties of any binary need to be confirmed by further observations. While even a deep ASKAP survey may not identify large numbers of new MSPs compared with the existing population, it would be competitive with existing all-sky surveys and could discover interesting new MSPs at high Galactic latitude without the need for computationally expensive all-sky periodicity searches.