Study of the Outer Galactic Structure for 288° <=l<=310° - 7° <=b<=2°

Details Study of the Outer Galactic Structure for 288° <=l<=310° - 7° <=b<=2° Study of the Outer Galactic Structure for 288° <=l<=310° - 7° <=b<=2°

Nov 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..25..207g&link_type=abstract

Astrophysics and Space Science, Volume 25, Issue 1, pp.207-216

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

The structure of the outer part of the Galaxy is studied, based upon 21-cm line observations of H i in the region 288°≤l≤310°, -7°≤b≤2°. In this longitude range the galactic plane is strongly bend toward negative latitudes. The principal outer structure is a spiral arm which has a pitch angle of 10° and is formed by several concentrations differing in shape and size. There exists also a secondary concentration which could be a split from the previous structure. Possible hypotheses about the origin of the later feature are discussed.

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