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EVIDENCE FOR PAST KNOT MERGERS IN THE HH34 JET
Within ≈30" from the outflow source, the HH34 jet has a chain of well aligned knots. The positions and proper motions of these knots can be used to determine dynamical timescales, and estimates of the ejection period (by taking differences between the dynamical timescales of the successive knot...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
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| Päätekijät: | , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2013
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| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57128966017 |
| Tagit: |
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