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The Jet/Counterjet Symmetry of the HH 212 Outflow

We present Spitzer (IRAC) images and a VLT 2.1 μm image of the HH 212 outow. We find that this outow has a strong symmetry, with jet/counterjet knot pairs with ∆x < 1´´ position offsets. We deduce that the jet/counterjet knots are ejected with time differences ∆τ0 ≈ 6 yr and velocity differences...

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Bibliografische gegevens
Gepubliceerd in:Revista Mexicana de Astronomía y Astrofísica
Hoofdauteurs: A. Noriega-Crespo, A. C. Raga, V. Lora, J. C. Rodríguez-Ramírez
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: Universidad Nacional Autónoma de México 2020
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Online toegang:https://www.redalyc.org/articulo.oa?id=57171642005
https://www.redalyc.org/journal/571/57171642005/
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