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Faint high{ionization arcs of emission are found to be associated with some of the proplyds in the Orion nebula. These arcs are typically o set by 0.5{4 arcsec from the proplyds, in the direction of the ionizing star (1 C Ori) and have commonly been interpreted as bowshocks, resulting from the collision between the transonic photoevaporating ow from the proplyd and the highly supersonic (1000 km s

Palabras clave: HYDRODYNAMICS | ISM: INDIVIDUAL (ORION NE- BULA) | ISM: JETS AND OUTFLOWS
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Universidad Autónoma del Estado de México
Sistema de Información Científica Redalyc ®
Versión 3.0 | 2017
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