Spectrophotometry in the galactic supernova remnants RCW 86, 103 and Kepler

Details Spectrophotometry in the galactic supernova remnants RCW 86, 103 and Kepler Spectrophotometry in the galactic supernova remnants RCW 86, 103 and Kepler

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204..273l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, July 1983, p. 273-287.

Other

69

Abundance, Emission Spectra, Interstellar Extinction, Milky Way Galaxy, Spectrophotometry, Supernova Remnants, Electron Density (Concentration), Forbidden Bands, H Lines, Line Shape, Shock Heating, Spectral Line Width

Scientific paper

The results of spectrophotometric observations in the galactic supernova remnants (SNR) RCW 86, 103 and Kepler are presented. The measurements were made with an angular resolution of about 4 arcsec in a number of different positions in each object. The authors also present the integrated spectra of the three remnants and compare them with the spectra of other galactic SNRs. The differential measurements reveal variations from point to point in the extinction towards the three objects, as well as in their intrinsic relative line-intensities. Some implications of the observed variations are discussed in the context of abundances and shock conditions.

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