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

Published online by Cambridge University Press:  14 August 2015

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

Extract

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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
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. 452454.Google Scholar