Optical spectrophotometry of the Cygnus Loop

Details Optical spectrophotometry of the Cygnus Loop Optical spectrophotometry of the Cygnus Loop

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sscr.conf..495f&link_type=abstract

In: Supernovae: A survey of current research; Proceedings of the Advanced Study Institute, Cambridge, England, June 29-July 10,

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Optical Emission Spectroscopy, Supernova Remnants, Astronomical Models, Emission Spectra, Line Spectra, Oxygen Ions, Radiant Flux Density, Shock Fronts, Spectral Energy Distribution, Visible Spectrum

Scientific paper

Cygnus Loop filament optical spectral properties are discussed, with emphasis on comparisons between observational and model data. Some line intensities are correlated among filaments in such a way as to suggest that a well resolved ionization structure behind the shock front is being observed. Departures from the steady flow condition assumed in the present model are found to be necessary in order to improve agreement with observations.

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