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Titlebook: Dense Molecular Gas around Protostars and in Galactic Nuclei; European Workshop on W.A. Baan,Y. Hagiwara,H.J. Langevelde Book 2005 Springer

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樓主: 叛亂分子
41#
發(fā)表于 2025-3-28 15:08:53 | 只看該作者
A Molecular Ring in the Liner NGC 5218entration with extensions out to a radius of 12″. The molecular mass detected is 2.4 × 10. . and the gas surface density is high, ~3000 . pc square in the inner 500 pc. The SFR is 2–3 . yr . and the SFE is ~13, which are low or moderate values for that gas surface density. We interpret the inner fea
42#
發(fā)表于 2025-3-28 20:15:22 | 只看該作者
43#
發(fā)表于 2025-3-29 00:57:43 | 只看該作者
discussed here are often in an early stage and undoubtedly their progress has bene?ted greatly from the opportunity to discuss results with the experts in a wide range of areas. Similarly, we feel con?dent tha978-90-481-6772-2978-1-4020-3831-0
44#
發(fā)表于 2025-3-29 03:52:19 | 只看該作者
Domestic Dog Cognition and Behavior activity. The overall lack of observational evidence for direct causal relationships between the presence of bars and interactions on the one hand, and starburst or Seyfert activity on the other could, however, easily be due to the possibility that we are not yet considering the correct spatial- or
45#
發(fā)表于 2025-3-29 10:37:13 | 只看該作者
https://doi.org/10.1007/978-3-642-53994-7ibution caused by orbit crowding effects. Based on these new data we have improved recent simulations of the warped disk in NGC3718. HE1029-1831 and 3C48 are nearby QSOs. HE10297-1831 is taken out of the Cologne nearby QSO sample. The maps of the integrated CO(1-0) and CO(2–1) emission clearly show
46#
發(fā)表于 2025-3-29 11:46:02 | 只看該作者
EVN Observations of H2O Masers Towards the High-Mass Young Stellar Object in AFGL 5142
47#
發(fā)表于 2025-3-29 15:42:36 | 只看該作者
Dense Molecular Gas around Protostars and in Galactic NucleiEuropean Workshop on
48#
發(fā)表于 2025-3-29 19:42:33 | 只看該作者
Dense Molecular Gas around Protostars and in Galactic Nuclei978-1-4020-3831-0
49#
發(fā)表于 2025-3-30 03:06:49 | 只看該作者
Gravitationally Induced Inflow in Starbursts and AGN activity. The overall lack of observational evidence for direct causal relationships between the presence of bars and interactions on the one hand, and starburst or Seyfert activity on the other could, however, easily be due to the possibility that we are not yet considering the correct spatial- or
50#
發(fā)表于 2025-3-30 05:16:00 | 只看該作者
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