Radio polarimetry of Galactic Centre pulsars - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2016

Radio polarimetry of Galactic Centre pulsars

D. H. F. M. Schnitzeler
  • Function : Author
R. P. Eatough
  • Function : Author
M. Kramer
  • Function : Author
K. J. Lee
  • Function : Author
A. Noutsos
  • Function : Author
R. M. Shannon
  • Function : Author


To study the strength and structure of the magnetic field in the Galactic Centre (GC), we measured Faraday rotation of the radio emission of pulsars which are seen towards the GC. Three of these pulsars have the largest rotation measures (RMs) observed in any Galactic object with the exception of Sgr A. Their large dispersion measures, RMs and the large RM variation between these pulsars and other known objects in the GC implies that the pulsars lie in the GC and are not merely seen in projection towards the GC. The large RMs of these pulsars indicate large line-of-sight magnetic field components between ∼ 16 and 33 μG; combined with recent model predictions for the strength of the magnetic field in the GC this implies that the large-scale magnetic field has a very small inclination angle with respect to the plane of the sky (∼12°). Foreground objects like the Radio Arc or possibly an ablated, ionized halo around the molecular cloud G0.11-0.11 could contribute to the large RMs of two of the pulsars. If these pulsars lie behind the Radio Arc or G0.11-0.11 then this proves that low-scattering corridors with lengths ≳100 pc must exist in the GC. This also suggests that future, sensitive observations will be able to detect additional pulsars in the GC. Finally, we show that the GC component in our most accurate electron density model oversimplifies structure in the GC.
Fichier principal
Vignette du fichier
stw841.pdf (831.08 Ko) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

insu-03669460 , version 1 (17-05-2022)



D. H. F. M. Schnitzeler, R. P. Eatough, K. Ferrière, M. Kramer, K. J. Lee, et al.. Radio polarimetry of Galactic Centre pulsars. Monthly Notices of the Royal Astronomical Society, 2016, 459, pp.3005-3011. ⟨10.1093/mnras/stw841⟩. ⟨insu-03669460⟩
14 View
8 Download



Gmail Facebook X LinkedIn More