Full description
We carried out a pilot FAST survey at intermediate Galactic latitudes and discovered five new pulsars (including two millisecond pulsars, MSPs). We confirmed all five pulsars and timed two pulsars (J1826-0049 and J1849+1000) during the 2022OCTS semester. A coherent timing solution was obtained for J1826-0049 (4.59 ms) and it is in a 6.7-day orbit with a white dwarf companion. The other pulsar, J1849+1000, turned out to be potentially exotic. While its large spin period variation can be fitted by a 26-day circular orbit with a massive companion, the residuals show strong quasi-periodic variations, which suggest the existence of a third object in an inner orbit. If confirmed, J1849+1000 will be in a stellar triple system with an outer orbit of 26 days and an inner orbit of a few days. This makes it potentially a unique system for tests of gravitational theories and understanding the formation and evolution of triple systems. Here we propose to continue our timing of J1826-0049 and J1849+1000. The goal is to refine our measurement of the parameters of J1826-0049 and understand the nature of J1849+1000Available: 2023-09-11
Data time period: 2023-04-01 to 2023-09-30
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Physical Sciences |
neutron stars |
pulsars |
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Identifiers
- DOI : 10.25919/JTYE-BG23
- Handle : 102.100.100/599571
- URL : data.csiro.au/collection/csiro:60279
