Non-circular motions in the galaxy as exhibited by very young stars
I. Expansion of the Gaseous and Stellar Components of the Galaxy If the gaseous component of the Galaxy is expanding as observed by Rougoor and Oort in the centre of the Galaxy and as postulated by Kerr in his early interpretation of spiral structure, the expansion must represent a phenomenon of fun...
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| Veröffentlicht in: | Symposium - International Astronomical Union 1964, Vol.20, p.92-99 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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