Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211..217b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 1, Feb. 1989, p. 217-229. Research supported by the Observatoire de H
Astronomy and Astrophysics
Astrophysics
12
Fabry-Perot Spectrometers, Forbidden Bands, Iron, Nebulae, Supernova Remnants, X Ray Sources, Astronomical Models, Brightness Distribution, Charge Coupled Devices, Cygnus Constellation, Emission Spectra, Ionization, Visible Spectrum
Scientific paper
We present results of a continuing program of observations of SNRs in the [Fe X] 6374 Å and [Fe XIV] 5303 Å coronal lines using the Fabry-Perot spectrophotometer of the Observatoire de Marseille. We have measured these lines at numerous places along the northeastern ridge of the Cygnus Loop. Our data generally agree with previously published brightnesses, obtained with non spectral techniques. The brightest [Fe X] features reach 5 10-7 erg cm-2 s-1 sr-1 averaged over 10 arcmin2. Evidence for line broadening (100 km s-1 FWHM) in a few bright fields is presented.
Ballet Jean
Caplan James
Dubreuil Didier
Rothenflug R.
Soutoul Aimé
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