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- W2064102009 abstract "Further spectrophotometric observations have been made of four filaments, and in particular detail of one filament, in the Cygnus Loop. The Balmer decrement for all of the filaments studied is 2.65, or radiative for case B The temperatures obtained from the line ratios for [0 iii] and [N ii] indicate that there is a stratification within individual filaments Collisional ionization may well be important in the high-temperature portions of the filaments, but high-temperature thermal radiation produces the ionization of the cooler parts of the filaments The so-called filaments are probably not filaments but irregular sheets produced by the collision of the advancing shock front with the clouds of the interstellar medium, seen edge on." @default.
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- W2064102009 date "1967-08-01" @default.
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- W2064102009 title "A Model for the filaments in the Cygnus Loop" @default.
- W2064102009 doi "https://doi.org/10.1086/149259" @default.
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