Projection effects in barred galaxies cause the wrong interpretation of radial flows
Galaxy disks in rotation are sometimes the site of radial flows, especially in their gas component. It is important to estimate the outflows, due to active galactic nucleus or supernovae feedback, or the inflows, due to bar gravity torques. However, these radial flows may be confused with noncircula...
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| Autors principals: | , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
EDP Sciences
2026-03-01
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| Col·lecció: | Astronomy & Astrophysics |
| Matèries: | |
| Accés en línia: | https://www.aanda.org/articles/aa/full_html/2026/03/aa58252-25/aa58252-25.html |
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