Modeling of IR emission of interstellar clouds. II. Self-consistent models of individual nearby clouds

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[1] MODELING OF IR EMISSION OF INTERSTELLAR CLOUDS .2. SELF-CONSISTENT MODELS OF INDIVIDUAL NEARBY CLOUDS
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[8] Polytropic models of filamentary interstellar clouds - II. Helical magnetic fields
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[9] Interstellar abundances in the Magellanic Clouds. II. The line of sight to SN 1987A in the large Magellanic Cloud
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[10] Self-consistent Models of Y Dwarf Atmospheres with Water Clouds and Disequilibrium Chemistry
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