SIMBAD references

2021MNRAS.501.1868C - Mon. Not. R. Astron. Soc., 501, 1868-1877 (2021/February-3)

Non-thermal filaments from the tidal destruction of clouds in the Galactic centre.

COUGHLIN E.R., NIXON C.J. and GINSBURG A.

Abstract (from CDS):

Synchrotron-emitting, non-thermal filaments (NTFs) have been observed near the Galactic centre for nearly four decades, yet their physical origin remains unclear. Here we investigate the possibility that NTFs are produced by the destruction of molecular clouds by the gravitational potential of the Galactic centre. We show that this model predicts the formation of a filamentary structure with length on the order of tens to hundreds of pc, a highly ordered magnetic field along the axis of the filament, and conditions conducive to magnetic reconnection that result in particle acceleration. This model therefore yields the observed magnetic properties of NTFs and a population of relativistic electrons, without the need to appeal to a dipolar, ∼mG, Galactic magnetic field. As the clouds can be both completely or partially disrupted, this model provides a means of establishing the connection between filamentary structures and molecular clouds that is observed in some, but not all, cases.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): black hole physics - hydrodynamics - magnetic fields - Galaxy: centre - Galaxy: kinematics and dynamics

Simbad objects: 5

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2021MNRAS.501.1868C and select 'bookmark this link' or equivalent in the popup menu


2021.12.09-15:56:09

© Université de Strasbourg/CNRS

    • Contact