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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
21#
發(fā)表于 2025-3-25 05:02:04 | 只看該作者
Clinton L. Beckford,Donovan R. Campbellspots are most likely associated with the tangentially seen parts of a nuclear accretion disk, while an association with dense warm gas interacting with the radio jets cannot yet be ruled out entirely.
22#
發(fā)表于 2025-3-25 07:53:01 | 只看該作者
Domestic Homicides and Death Reviewst evolution. The discussion on the interpretation of HNC 1-0 emission includes the importance of ion-neutral chemistry in a luminous starburst region. Finally, simple cartoon ISM models and how they can be applied to LIRGs and ULIRGs, are presented.
23#
發(fā)表于 2025-3-25 14:59:59 | 只看該作者
24#
發(fā)表于 2025-3-25 15:48:05 | 只看該作者
25#
發(fā)表于 2025-3-25 21:25:45 | 只看該作者
26#
發(fā)表于 2025-3-26 03:19:16 | 只看該作者
27#
發(fā)表于 2025-3-26 05:44:31 | 只看該作者
Outflow, Infall, and Rotation in High-Mass Star Forming Regionsn pressure should reverse the infall thus preventing further growth of the stellar mass. After illustrating the two models proposed to solve this problem (“accretion” and “coalescence”), we review the observational evidence pro/contra such models, focusing on the kinematics of the molecular gas wher
28#
發(fā)表于 2025-3-26 10:33:21 | 只看該作者
MERLIN and Puschino Observations of H2O Masers in Outer Galactic SFR S128N from the Puschino radio telescope. The drift velocities of the masers and the velocity and location of a new maser region add depth to the model of two colliding CO clouds triggering collapse. Some H.O masers appear to originate directly from this shock front. The brightest maser appears typical of
29#
發(fā)表于 2025-3-26 16:09:53 | 只看該作者
30#
發(fā)表于 2025-3-26 17:25:20 | 只看該作者
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