Temperature and Kinematics of C [CSC]iv[/CSC] Absorption Systems
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چکیده
منابع مشابه
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The metal line profiles of different ions observed in high H i column density systems [N(H i) > 10 cm] in quasar spectra can be used to constrain the ionization structure and kinematic characteristics of the absorbers. For these purposes, a modified Monte Carlo Inversion (MCI) procedure was applied to the study of three absorption systems in the spectrum of the HDF-South quasar J2233–606 obtain...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 1996
ISSN: 0004-637X
DOI: 10.1086/310187