Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-12T19:42:22.044Z Has data issue: false hasContentIssue false
  • English
  • Français

A mechanism for the origin and development of spiral arms in a galaxy

Published online by Cambridge University Press:  14 August 2015

Paris Pişmiş
Paris Pişmiş*
Affiliation:
Instituto de Astronomía Universidad Nacional Autónoma de México

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is generally believed that the constituents of a galaxy like ours are formed from an isolated gaseous assembly at successive stages, starting from a spheroidal sybsystem down to the flattest subsystem.

Type
III. SPIRAL STRUCTURE
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 145 - 146
Copyright
Copyright © Reidel 1979 

References

Henderson, A. P.: 1967, , .Google Scholar
Huang, S. S., and Pişmiş, P.: 1960, Bol. Obs. Tonantzintla Tacubaya 2, 7.Google Scholar
Pişmiş, P.: 1960, Bol. Obs. Tonantzintla Tacubaya 2, 3.Google Scholar
Pişmiş, P.: 1961, Bol. Obs. Tonantzintla Tacubaya 3, 3.Google Scholar
Pişmiş, P.: 1963, Bol. Obs. Tonantzintla Tacubaya 3, 127.Google Scholar
Pişmiş, P.: 1968, Bol. Obs. Tonantzintla Tacubaya 4, 229.Google Scholar
Pişmiş, P.: 1970, in IAU Symposium No. 38, ed. Becker, W. and Contopoulos, G. (Dordrecht: Reidel) pp. 452–454.Google Scholar