Herbig-Haro Objects from Orbiting Sources

Details Herbig-Haro Objects from Orbiting Sources Herbig-Haro Objects from Orbiting Sources

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..140m&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

1

Ism: Jets And Outflows, Stars: Pre-Main Sequence

Scientific paper

The wiggles detected in HH outflows can be related, in a few cases, to the orbital motion of a binary stellar system. For these outflows it is possible to calculate the mass of the jet source and the orbital parameters using observational measurements (i.e., the opening angle of the wiggling jet pattern, the separation between successive wiggles, the jet velocity and the orientation of the jet with respect to the plane of the sky). An application to a few real cases will be presented.

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