Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-29T07:51:39.829Z Has data issue: false hasContentIssue false

Large-scale structure and kinematics of the Galactic System

Published online by Cambridge University Press:  14 August 2015

B. Lindblad*
Affiliation:
Stockholms Observatorium

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, I believe, of fundamental importance to find out how far the structure and motions in the galaxies can be explained by gravitational theory. This does not deny that hydrodynamic and electromagnetic forces may play an important part. The special point which I have in mind is the possibility, from the standpoint of gravitational theory, for the spiral structure to be a kind of quasi-steady state of comparatively long lifetime.

Type
Section 1: The Galaxy
Copyright
Copyright © Australian Academy of Science 1964 

References

Elvius, A. (1958).— Pop. Astron. Tidskr. 39: 151.Google Scholar
Elvius, A., and Herlofson, N. (1960).— Ap.J. 131: 304–9 (= Uppsala Obs. Medd. No. 128.).Google Scholar
Elvius, A., and Lindblad, P. O. (1959).— Arkiv Astron. 2: 393406 (= Uppsala Obs. Medd. No. 126.).Google Scholar
Höglund, B. (1963).— Arkiv Astron. 3: 215–72.Google Scholar
Lindblad, B. (1958).— Stockholms Obs. Annaler 20: No. 4.Google Scholar
Lindblad, B. (1963).— Stockholms Obs. Annaler 22: No. 5.Google Scholar
Lindblad, P. O. (1960a).— Stockholms Obs. Annaler 21: No. 4.Google Scholar
Lindblad, P. O. (1960b).— Pop. Astron. Tidskr. 41: 132–49.Google Scholar
Mayall, N. U. (1960).—Colloque Int. CNRS. [Paris 1959] Ann. d'Ast. 23: 344–59.Google Scholar
Ramberg, J. M. (1957).— Stockholms Obs. Annaler 20: No. 1.Google Scholar