The Spiral Wave of Our Galaxy Near Inner Lindblad Resonance
The dispersion relationship for short-wavelength spiral density waves in our Galaxy has been refined to remove the divergences that occurred in wave number and in amplitude as inner Lindblad resonance is approached. The wave is found to be evanescent in an annular region near 4 kpc. By 3 kpc, the in...
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| Veröffentlicht in: | Proc Natl Acad Sci U S A |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
National Academy of Sciences
1971
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| Online-Zugang: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC389359/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16591941/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.68.9.2095 |
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