Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991natur.354..121c&link_type=abstract
Nature (ISSN 0028-0836), vol. 354, Nov. 14, 1991, p. 121-124. Research supported by NSF and NASA.
Astronomy and Astrophysics
Astronomy
116
Electron Density (Concentration), Electron Distribution, Free Electrons, Milky Way Galaxy, Spatial Distribution, Extragalactic Radio Sources, Interstellar Matter, Ionized Gases, Massive Stars, Pulsars, Stellar Winds
Scientific paper
Various radioastronomical measurements are synthesized here to derive a large-scale Galactic model for the distribution of free electrons and for microstructure in the distribution that seems to be caused by turbulence in the ISM. A two-component axisymmetric model fitted on all scales from 100 km to a few pc, accounts for most of the data. A population of dense, discrete clouds is also needed, and there is some evidence for spiral structure. The model allows better distance estimates for pulsars to be made. The implications of the model for the structure and ionization of the ISM and for the distribution of interstellar turbulence and the diffusion of cosmic rays are discussed.
Cordes James M.
Frail Dale A.
Ryan Mark
Spangler Steven R.
Weisberg Joel M.
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