Star Formation Regions: HH1

Computer Science

Scientific paper

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Hst Proposal Id #2897

Scientific paper

An image will be taken of HH1 using the F/96 camera of the FOC and F190M filter. This object consists of at least six semi-stellar knots wrapped in a common nebular envelope. These knots appear to be caused by the interaction of a jet from a central star about 25 arcsec away from HH1. The resulting images will be compared with existing ground-based data and used to show the interaction of a jet or stellar wind with a dense instellar medium and explore the possibility that we are looking at an environment of star-formation.

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