Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aj....109..752i&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 109, no. 2, p. 752-761
Astronomy and Astrophysics
Astronomy
10
Astronomical Models, Electron Density (Concentration), Electron Energy, Flux Density, Herbig-Haro Objects, Position (Location), Velocity, Carbon, H Alpha Line, Kinematics, Line Spectra, Mathematical Models, Oxygen, Shock Waves, Sulfur
Scientific paper
Many features of Herbig-Haro objects can be reproduced using a kinematical bow shock model. We use the model to generate position-velocity (PV) diagrams of flux in H-alpha (O I) lambda lambda 6300+63, (S II) lambda lambda 6716+31, (O III) lambda lambda 4959+5007, and (C I) lambda lambda 9823+50, line ratios of (O I)/H-alpha, (O I)/(S II), (S II)/H-alpha, H-alpha(S II), and (O III)/H-alpha, electron density Ne, and electron temperature Te. We show how position-velocity diagrams of Ne and flux vary with shock velocity. By matching the diagrams from single lines, the line ratios, and Ne with observations, we determined a narrow range of shock parameters for HH 1F, 2(A' + H), and 43 (B + C). We model the Ne features of HH 2(A' + H) as a superposition of two bowshocks. We also show that the effects of slight misalignments of the two diagrams to be divided can produce artifacts in the line ratios and Ne which obliterate the physical features. We show that Ne in HH 1 can only be explained using the kinematical model by taking these misalignments into account.
Indebetouw Remy
Noriega-Crespo Alberto
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