Evidence for evaporation around the filamentary structure in the Cygnus Loop

Details Evidence for evaporation around the filamentary structure in the Cygnus Loop Evidence for evaporation around the filamentary structure in the Cygnus Loop

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...133..357b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 133, no. 2, April 1984, p. 357-362.

Astronomy and Astrophysics

Astrophysics

8

Atmospheric Models, Supernova Remnants, Supernovae, X Ray Sources, Emissivity, Ionization, Iron, Line Spectra

Scientific paper

The structure of the north-east part of the Cygnus Loop in the Fe X and Fe XIV coronal lines is compared with X-ray maps. The intensity variations in the Fe X line exclude a simple Sedov solution. Emission from the transition medium around evaporating cool clouds associated with the optical filaments can explain the Fe X profile. More realistic models are considered.

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