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High-Resolution Radial Velocity Mapping of Optical Filaments in Evolved Supernova Remnants
Published online by Cambridge University Press: 12 April 2016
Abstract
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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
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 443 - 446
- Copyright
- Copyright © Cambridge University Press 1988
References
Boksenberg,
1972, Auxiliary Instrumentation for Large Telescopes, Proc. of ESO/CERN Conf. Geneva, p. 205.Google Scholar
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