Hostname: page-component-7bb8b95d7b-2h6rp Total loading time: 0 Render date: 2024-09-12T08:11:10.603Z Has data issue: false hasContentIssue false
  • English
  • Français

Kinematics of Supernova Remnants in the Galaxy and LMC

Published online by Cambridge University Press:  04 August 2017

Peter Shull Jr.
Peter Shull Jr.*
Affiliation:
Max-Planck-Institut für Astronomie and Rice University

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The optical emission lines of six SNRs have been observed at very high angular and kinematic resolutions. Kinematic ion temperatures were derived, and evidence was found in shocked regions for Maxwellian microturbulence on scales ≤ 0.01 pc, and for non-Maxwellian macroturbulence on scales > 0.1 pc. The widths of shocked regions in the Cygnus Loop and the existence of three types of spectral feature in the LMC remnants are discussed in terms of SNR evolution in cloudy interstellar media.

Type
II. Middle Aged and Older Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 295 - 298
Copyright
Copyright © Reidel 1983 

References

Cox, D.P.: 1979, Astrophy. J., 234, p. 863.Google Scholar
Falk, S.W.: 1978, Astrophys.J.Lett., 225, p. L133.Google Scholar
Shull, J.M., and McKee, C.F.: 1979, Astrophys.J., 227, p. 131.Google Scholar
Shull, P. Jr.: 1982, Astrophys.J., 253, p. 682.Google Scholar