Discovery of Three New Millisecond Pulsars in Terzan 5

Authors
  • M. Cadelano
  • S.M. Ransom
  • P.C.C. Freire
  • F.R. Ferraro
Publication date 2018
Journal Astrophysical Journal
Article number 125
Volume | Issue number 855 | 2
Number of pages 7
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
We report on the discovery of three new millisecond pulsars (MSPs; namely J1748−2446aj, J1748−2446ak, and J1748−2446al) in the inner regions of the dense stellar system Terzan 5. These pulsars have been discovered thanks to a method, alternative to the classical search routines, that exploited the large set of archival observations of Terzan 5 acquired with the Green Bank Telescope over five years (from 2010 to 2015). This technique allowed the analysis of stacked power spectra obtained by combining ~206 hr of observation. J1748−2446aj has a spin period of ~2.96 ms, J1748−2446ak of ~1.89 ms (thus it is the fourth fastest pulsar in the cluster) and J1748−2446al of ~5.95 ms. All three MSPs are isolated, and currently we have timing solutions only for J1748−2446aj and J1748−2446ak. For these two systems, we evaluated the contribution to the measured spin-down rate of the acceleration due to the cluster potential field, thus estimating the intrinsic spin-down rates, which are in agreement with those typically measured for MSPs in globular clusters (GCs). Our results increase the number of pulsars known in Terzan 5 to 37, which now hosts 25% of the entire pulsar population identified, so far, in GCs.
Document type Article
Language English
Published at https://doi.org/10.3847/1538-4357/aaac2a
Other links http://adsabs.harvard.edu/abs/2018ApJ...855..125C
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