Voyager spectral observations of the Cygnus Loop nebula, 600-1700 A

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Line Spectra, Nebulae, Ultraviolet Spectrometers, Voyager Project, Brightness, Interstellar Matter, Observations, Voyager 2, Ultraviolet, Spectrometers, Emissions, Wavelengths, Spectrum, Plasmas, Brightness, Supernova, Radiation, Cygnus Loop, Nebulas, Continuum

Scientific paper

Observations of the Cygnus Loop objects NGC 6995 and NGC 6992, which are defined by bright filamentary structure in visible radiation, are reported which were made with the Voyager 2 UV spectrometer in the wavelength range from 600 to 1700 A. The results are compared with far-UV observations performed during the Apollo 16 mission. It is found that measurable emission in the region from 912 to 1050 A is sharply confined to the location of the optical filaments, that emissions in the range from 1200 to 1680 A exhibit a sharp decline 0.5 deg of arc west of the filaments toward the center of the Loop, and that the most likely emissions in the 912-1050-A region are C II at 1037 A, C III at 977 A, and O I at 936 and 999.5 A. The results suggest that the radiation in the 912-1050-A range is associated with cooler postshock regions and that the shock velocities range from 70 to 100 km/s

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