Hostname: page-component-848d4c4894-ttngx Total loading time: 0 Render date: 2024-05-06T18:58:23.431Z Has data issue: false hasContentIssue false

High-Resolution Radial Velocity Mapping of Optical Filaments in Evolved Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

H. Greidanus
Affiliation:
Sterrewacht Leiden, The Netherlands
R.G. Strom
Affiliation:
Netherlands Foundation for Radio Astronomy

Abstract

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.

We report on observations of the kinematical structure of optical filaments in evolved supernova remnants, using an imaging Fabry-Perot interferometer. The radial velocity characteristics as seen in [OIII] λ5007 emission in one area in the Cygnus Loop are described, where four kinematically different components contributing to the emission can be recognized.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1988

References

Atherton, et al. 1982, M.N.R.A.S. 201, 661.Google Scholar
Boksenberg, 1972, Auxiliary Instrumentation for Large Telescopes, Proc. of ESO/CERN Conf. Geneva, p. 205.Google Scholar
Hester, 1987, Astroph. J. 314, 187.Google Scholar