An Ionized Microjet from the Orion Nebula Proplyd LV 2

Details An Ionized Microjet from the Orion Nebula Proplyd LV 2 An Ionized Microjet from the Orion Nebula Proplyd LV 2

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..13...59h&link_type=abstract

Emission Lines from Jet Flows (Eds. W. J. Henney, W. Steffen, A. C. Raga, and L. Binette) Revista Mexicana de Astronomía y Astro

Other

H Ii Regions, Ism: Jets And Outflows, Stars: Pre-Main Sequence, Stars: Mass Loss

Scientific paper

We present results of multi-wavelength observations of the Orion nebula proplyd LV 2 (M42 167-317), concentrating on our analysis of the microjet that emerges from the proplyd's ionization front. The microjet is one-sided at its base but faint, symmetrical jet filaments are seen on both sides at arcsecond scales. The physical characteristics of the jet (opening angle, density, mass-loss rate, momentum-loss rate, luminosity) are estimated from the observations and compared with those of other irradiated microjets.

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