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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...

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Foilsithe in:Revista Mexicana de Astronomía y Astrofísica
Main Authors: A. C. Raga, A. Noriega-Crespo
Formáid: Artigo
Teanga:Inglês
Foilsithe: Universidad Nacional Autónoma de México 2013
Ábhair:
ISM
Rochtain Ar Líne:https://www.redalyc.org/articulo.oa?id=57128966017
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