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- W44819723 abstract "From observation of the galactic structure in Cygnus, the system of filamentary nebulae was found to lie at a distance of roughly 1.5 kpc, in the same region as about half the thermal radio sources in Cygnus X, the supernova remnant near gamma Cygni, and the association Cygnus OB2, in the direction of which the X-ray source Cygnus XR-3 is observed. The source of excitation was probably the pulse of radiation from a supernova explosion, as proposed in the case of Gum nebula. However continuing excitation by early stars in the region of Cygnus X cannot be excluded." @default.
- W44819723 created "2016-06-24" @default.
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- W44819723 date "1971-09-01" @default.
- W44819723 modified "2023-09-27" @default.
- W44819723 title "A discussion of the H-alpha filamentary nebulae and galactic structure in the Cygnus region" @default.
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- W44819723 hasPublicationYear "1971" @default.
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