SARA BONITO
2005
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2-D Hydrodynamics of Protostellar Jet Interaction with Interstellar
Medium (M = 300; na/nj = 10) with Thermal Conduction and Radiative Losses taken into account: Temperature (on the left) and density (on the right) in a linear scale
R.Bonito
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2-D Hydrodynamics of Protostellar Jet Interaction with Interstellar
Medium (M = 300; na/nj = 10) with Thermal Conduction and Radiative Losses taken into account: Temperature (on the left) and density (on the right)
R.Bonito
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2-D Maps of Protostellar Jet Interaction with Interstellar
Medium (M = 300; na/nj = 10) with Thermal Conduction and Radiative Losses taken into account: Temperature (upper panels on the left), density (upper panels on the right) and X-ray Emission as predicted to be observed with Chandra/ACIS-I (lower panels)
Adapted from R. Bonito, S. Orlando, G. Peres, F. Favata, R. Rosner 2004, X-ray emission mechanisms in protostellar jets, oral presentation, PROC. 13th Cool Stars Workshop, Hamburg, 5-9 July 2004, F. Favata ed.
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2-D Zoom of Protostellar Jet Interaction with Interstellar
Medium (M = 300; na/nj = 10) with Thermal Conduction and Radiative Losses taken into account: Temperature (on the left), density (on the right) in a linear scale
Adapted from R. Bonito, S. Orlando, G. Peres, F. Favata, R. Rosner 2004, X-ray emission mechanisms in protostellar jets, oral presentation, PROC. 13th Cool Stars Workshop, Hamburg, 5-9 July 2004, F. Favata ed.