Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.293...27r&link_type=abstract
Astrophysics and Space Science, v. 293, Issue 1, p. 27-36 (2004).
Astronomy and Astrophysics
Astrophysics
2
Ism:, Herbig-Haro Objects, Jets And Outflows, Kinematics And Dynamics, Shock Waves
Scientific paper
This paper reviews the numerical simulations of radiative jets with concrete predictions of the emitted radiation, which can be compared directly with observations of individual HH objects. The only models that have been developed to this point are the “internal working surface model” (in which the structures along HH jets are interpreted as working surfaces resulting from a time-variability in the ejection) or the “Kelvin-Helmholtz instability model” (in which the HH knots are associated with shocks resulting from K-H instabilities in the jet beam/environment boundary). The predictions of intensity maps, line ratios, line profiles and proper motions are discussed.
Beck Terry
Raga Alejandro C.
Riera Arnau
No associations
LandOfFree
Interpreting the Observations of Herbig-Haro Jets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Interpreting the Observations of Herbig-Haro Jets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interpreting the Observations of Herbig-Haro Jets will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1061222