New features in the local spiral structure

Details New features in the local spiral structure New features in the local spiral structure

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..666d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Nov. 1981, p. 666-670.) Soviet Astronomy Letters, vol. 7, Nov.-Dec. 1981, p. 370-372

Astronomy and Astrophysics

Astronomy

2

Galactic Structure, Milky Way Galaxy, Stellar Evolution, Supernova Remnants, X Ray Sources, Astronomical Models, Chemical Composition, Gamma Ray Astronomy, H I Regions, Spatial Distribution

Scientific paper

Groups (or complexes) of star formation regions, concentrations of H I regions, supernova remnants, and X-ray and gamma-ray sources located in the local spiral arm are treated as constituents of more intricate complexes of interrelated objects: interarm superassociations. These complexes differ in their position relative to the structural features of the local arm, in their structure and composition, and in the direction along which star formation is propagated through them. New transverse offshoots are outlined, forming interarm links along l = 120-300 degrees.

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