scholarly journals Observational Evidence for Galactic Spiral Structure

1971 ◽  
pp. 63-87 ◽  
Author(s):  
Bart J. Bok
1971 ◽  
Vol 2 ◽  
pp. 63-87 ◽  
Author(s):  
Bart J. Bok

Does our Galaxy possess spiral structure and, if so, can this structure be traced observationally with some degree of confidence? This is the major question to which I shall address myself tonight. Following my talk, Professor Lin will speak about the theoretical aspects of spiral structure. I shall be very brief in my references to spiral structure in galaxies outside our own and leave it largely to Professor Lin to speak about observations on other spiral galaxies and their relevance for possible theoretical interpretations.A year ago, my good and distinguished friend Professor B. A. Vorontsov-Velyaminov chided me in his address at the Basel Symposium for having been too eager to accept the fact that observation suggests that our Galaxy really possesses spiral structure. I hope to show in my Discourse that for our Galaxy we have indeed evidence for the presence of an underlying structure of spiral features.


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.


2019 ◽  
Vol 487 (1) ◽  
pp. 1400-1409 ◽  
Author(s):  
B-Q Chen ◽  
Y Huang ◽  
L-G Hou ◽  
H Tian ◽  
G-X Li ◽  
...  

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