The HH111 jet and multiple outflow episodes from young stars

Details The HH111 jet and multiple outflow episodes from young stars The HH111 jet and multiple outflow episodes from young stars

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.340...42r&link_type=abstract

Nature (ISSN 0028-0836), vol. 340, July 6, 1989, p. 42-45.

Astronomy and Astrophysics

Astronomy

143

Early Stars, Gas Jets, Herbig-Haro Objects, Orion Nebula, Stellar Mass Accretion, Astronomical Maps, Infrared Sources (Astronomy), Molecular Clouds, Shock Waves

Scientific paper

The discovery of an exceptionally fine jet, HH111, emerging from a young star still embedded in the Orion molecular clouds, is reported. The jet system displays four bow-shock-like features moving in pairs in opposite directions from a 25-solar luminosity infrared source. With an extent of more than 0.8 parsec, HH111 is the largest bipolar Herbig-Haro flow known. It is argued that such jets are highly transient phenomena that are related to eruptive accretion events in the buildup of the central star.

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