继承人 发表于 2025-3-30 10:25:47

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enhance 发表于 2025-3-30 13:19:51

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

舔食 发表于 2025-3-30 20:29:19

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Hormones 发表于 2025-3-30 23:36:35

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commensurate 发表于 2025-3-31 03:13:12

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天然热喷泉 发表于 2025-3-31 06:58:08

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justify 发表于 2025-3-31 11:53:57

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

不成比例 发表于 2025-3-31 13:52:33

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绿州 发表于 2025-3-31 17:39:36

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有帮助 发表于 2025-4-1 00:16:42

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