Ultraviolet spectra of the Cygnus Loop - Depletion of the heavy elements

Details Ultraviolet spectra of the Cygnus Loop - Depletion of the heavy elements Ultraviolet spectra of the Cygnus Loop - Depletion of the heavy elements

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85..203c&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 203-219.

Astronomy and Astrophysics

Astronomy

11

Abundance, Cygnus Constellation, Heavy Elements, Ultraviolet Astronomy, Ultraviolet Spectra, Carbon, H Beta Line, Oxygen Spectra, Propagation Velocity, Shock Wave Propagation

Scientific paper

A comparison between the observed UV spectra and detailed consistent
calculations of the Cygnus Loop (CL) is presented. It is shown that the
spectra can be explained by assuming that the CL moves into a fully
ionized gas. The forbidden O III/H-beta ratio is shown to be an
indicator of the fraction of He(2+) in the gas entering the shock.

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