Modeling the Radial Velocities and Proper Motions of Herbig-Haro Objects

Details Modeling the Radial Velocities and Proper Motions of Herbig-Haro Objects Modeling the Radial Velocities and Proper Motions of Herbig-Haro Objects

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..13...79r&link_type=abstract

Emission Lines from Jet Flows, Isla Mujeres, Q.R., México, November 13-17, 2000 (Eds. W. J. Henney, W. Steffen, A. C. Raga, and

Astronomy and Astrophysics

Astronomy

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

Scientific paper

This paper discusses the different approaches that have been used for modeling the emission of Herbig-Haro (HH) objects. Even though axisymmetric or 3D simulations have been carried out for modeling specific objects, most comparisons carried out between theory and observations have been based on the use of simple, analytic descriptions of the kinematical structure of jets. These analytic models are summarized and some new possibilities are discussed.

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