scholarly journals The Galactic spiral structure as revealed by O- and early B-type stars

2019 ◽  
Vol 487 (1) ◽  
pp. 1400-1409 ◽  
Author(s):  
B-Q Chen ◽  
Y Huang ◽  
L-G Hou ◽  
H Tian ◽  
G-X Li ◽  
...  
1970 ◽  
Vol 38 ◽  
pp. 189-198 ◽  
Author(s):  
S. W. McCuskey

Aside from the well-known spiral arm tracers such as the OB associations, young galactic clusters, WR stars and possibly the long-period classical cepheids, the more common stars in the neighborhood of the sun within 2 kpc show little or no relationship to the local spiral structure of the galaxy.


1970 ◽  
Vol 38 ◽  
pp. 228-231
Author(s):  
T. A. Uranova

A maximum of dust density along the inner edge of the Cygnus arm is found. It seems that the same happens along the inner edges of the Perseus and the Sagittarius arms.


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