Titlebook: Dusty Objects in the Universe; Proceedings of the F E. Bussoletti,A. A. Vittone Conference proceedings 1990 Kluwer Academic Publishers 1990

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Shuichi Kurabayashi,Hiroki Hanaokahe carbon dust were observed when the pressure of the quenching gas was increased. At low pressures (order 10 torr), the spectra show the familiar broad continua. At high pressures (order 100 torr), narrow lines in the IR and two (or possibly three) broad features in the UV emerge. The four stronges

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A Hybrid Approach of HTTP Anomaly Detectiondicate that the bulk of the gas is confined to the optical dust lane but that the far-IR emission has a significantly greater scale height. We conclude from a comparison of these two data sets that there is a substantial amount of cool dust present in Centauras A which is not intimately associated w

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