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• W4301235096 abstract "Context. In the interpretation of stellar jet observations, the physical parameters are usually determined from emission line ratios, obtained from spectroscopic observations or using the information contained in narrow band images. The basic hypothesis in the interpretation of the observations is that the emitting region is homogeneous along the line of sight. Actually, stellar jets are in general not homogeneous, and therefore line of sight convolution effects may lead to the main uncertainty in the determination of the physical parameters." @default.
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• W4301235096 date "2008-05-06" @default.
• W4301235096 modified "2023-09-27" @default.
• W4301235096 title "Diagnostics of inhomogeneous stellar jets" @default.
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• W4301235096 doi "https://doi.org/10.1051/0004-6361:200809621" @default.
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