Keywords
Astronomical Models
Continuous Spectra
Herbig-Haro Objects
Radio Emission
Shock Waves
Thermal Emission
Brightness Temperature
Radio Sources (Astronomy)
Radio Spectra
X Ray Sources
Astrophysics
Herbig-Haro Objects:Radio Radiation
Herbig-Haro Objects:Shock Waves
Radio Radiation:Herbig-Haro Objects
Radio Radiation:Shock Waves
Shock Waves:Herbig-Haro Objects
Shock Waves:Radio Radiation
Continuous Spectra
Herbig-Haro Objects
Radio Emission
Shock Waves
Thermal Emission
Brightness Temperature
Radio Sources (Astronomy)
Radio Spectra
X Ray Sources
Astrophysics
Herbig-Haro Objects:Radio Radiation
Herbig-Haro Objects:Shock Waves
Radio Radiation:Herbig-Haro Objects
Radio Radiation:Shock Waves
Shock Waves:Herbig-Haro Objects
Shock Waves:Radio Radiation
How to Cite
A model for the thermal radio continuum emission produced by a shock wave and its application to the Herbig-Haro objects 1 and 2. (1987). Revista Mexicana De Astronomía Y Astrofísica, 14(1), 595-602. https://astronomia.unam.mx/journals/rmxaa/article/view/1987rmxaa..14..595c
Abstract
The present model for the thermal radio continuum emission produced by a shock wave is applied to Pravdo et al.'s (1985) observations at 2, 6, and 20 cm of the HH1-2 system. The spectrum thus obtained is similar to those known in H II regions and can reproduce the HH1-2 spectra; the observed spectrum of the central (and possibly exciting) source, however, can be only partially reproduced. These results suggest that the radio emission of the central source is not produced by a shock wave.Similar Articles
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