Distinctive structural features in the local spiral arm

Details Distinctive structural features in the local spiral arm Distinctive structural features in the local spiral arm

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..745d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Nov.-Dec. 1980, p. 745-749.) Soviet Astronomy Letters, vol. 6, Nov.-Dec. 1980, p. 39

Astronomy and Astrophysics

Astronomy

1

Galactic Structure, Milky Way Galaxy, Spiral Galaxies, Supernova Remnants, Astronomical Maps, Astronomical Models, Nebulae

Scientific paper

The structural properties of two local features of the Orion galactic spiral arm close to the sun, i.e., the Gould and de Vaucouleurs Belt, are discussed. Analysis of data on possible supernova remnants indicates that parts of these features are arrayed in thin, flat layers inclined at various angles to the galactic plane. The objects comprising these structural features are typically distributed in the form of clouds, rings, or shells.

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