A Herbig-Haro object in NGC 3603?

Details A Herbig-Haro object in NGC 3603? A Herbig-Haro object in NGC 3603?

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.231p..33c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 231, March 15, 1988, p. 33p-37p. SERC-supported researc

Astronomy and Astrophysics

Astronomy

3

Herbig-Haro Objects, Hydrogen Clouds, Plasma Jets, Stellar Winds, Astronomical Maps, Energy Sources, Flow Velocity, Ionized Gases

Scientific paper

A jet of material has been discovered emerging from an ionized knot in the core of NGC 3603 with a relative velocity of ≡110 km s-1. The central OB cluster is not thought to be the energy source of this phenomenon even though the knot lies on the edge of the wind-driven bubble surrounding the cluster. Instead a wind-producing star embedded in the nearby infrared source IRS1 is considered a more likely candidate. The presence of an energy source within the knot itself, however, is also a possibility.

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