Abstract:
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. © 1973 D. Reidel Publishing Company.
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Citas:
---------- APA ----------
Garzoli, S.L. & Mirabel, I.F.
(1973)
. Study of the outer galactic structure for 288°≤l≤310°, -7°≤b≤2°. Astrophysics and Space Science, 25(1), 207-216.
http://dx.doi.org/10.1007/BF00648235---------- CHICAGO ----------
Garzoli, S.L., Mirabel, I.F.
"Study of the outer galactic structure for 288°≤l≤310°, -7°≤b≤2°"
. Astrophysics and Space Science 25, no. 1
(1973) : 207-216.
http://dx.doi.org/10.1007/BF00648235---------- MLA ----------
Garzoli, S.L., Mirabel, I.F.
"Study of the outer galactic structure for 288°≤l≤310°, -7°≤b≤2°"
. Astrophysics and Space Science, vol. 25, no. 1, 1973, pp. 207-216.
http://dx.doi.org/10.1007/BF00648235---------- VANCOUVER ----------
Garzoli, S.L., Mirabel, I.F. Study of the outer galactic structure for 288°≤l≤310°, -7°≤b≤2°. Astrophys Space Sci. 1973;25(1):207-216.
http://dx.doi.org/10.1007/BF00648235