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Titlebook: Astrophysics in the Next Decade; The James Webb Space Harley A. Thronson,Massimo Stiavelli,Alexander Tie Conference proceedings 2009 Spring

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樓主: 萬(wàn)靈藥
41#
發(fā)表于 2025-3-28 15:01:01 | 只看該作者
42#
發(fā)表于 2025-3-28 21:39:56 | 只看該作者
Flex with Photoshop and Illustrator,will discuss the main options for using JWST and concurrent facilities to study the early, gas-rich, massive phases of protoplanetary disks. We discuss the opportunities to study gas and dust in such disks and to derive constraints on physical and chemical processes taking place there.
43#
發(fā)表于 2025-3-29 00:14:17 | 只看該作者
https://doi.org/10.1007/978-1-4020-9457-6Accretion; Exoplanet discovery; Galaxy Evolution; Hubble successor; JWST; James Webb Space Telescope; Reds
44#
發(fā)表于 2025-3-29 06:38:34 | 只看該作者
978-90-481-8132-2Springer Science+Business Media B.V. 2009
45#
發(fā)表于 2025-3-29 10:32:26 | 只看該作者
Accretion Disks Before (?) the Main Planet Formation Phase,will discuss the main options for using JWST and concurrent facilities to study the early, gas-rich, massive phases of protoplanetary disks. We discuss the opportunities to study gas and dust in such disks and to derive constraints on physical and chemical processes taking place there.
46#
發(fā)表于 2025-3-29 12:22:33 | 只看該作者
47#
發(fā)表于 2025-3-29 19:21:15 | 只看該作者
Flex Video Gallery with Drag-and-Drop,nsitivity of ALMA, Herschel, SOFIA, JWST and ELTs across the full range of wavelengths from cm to μm will be essential to trace this lifecycle of gas and dust from clouds to planets. The continued need for basic molecular data on gaseous and solid-state material coupled with powerful radiative trans
48#
發(fā)表于 2025-3-29 20:41:18 | 只看該作者
49#
發(fā)表于 2025-3-30 00:44:01 | 只看該作者
50#
發(fā)表于 2025-3-30 07:18:31 | 只看該作者
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