草率男
发表于 2025-3-25 07:03:24
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NATTY
发表于 2025-3-25 09:42:10
Protostellar Jets: A High Angular Resolution Perspectiveery recently, puts us in a very good position to plan rich and fruitful observative campaigns with the instruments being developed for astronomy at IR, submm amd mm wavelengths, in interferometric or single-telescope modes.
悠然
发表于 2025-3-25 11:41:56
Pre-Main-Sequence Evolutionand Brown Dwarfs Beyond the Solar Vicinityd is not affected by the problems mentioned above, which makes it a privileged target for studying not only PMS evolution and BDs but also offers a valuable opportunity to study the IMF well down into the substellar regime.
大量杀死
发表于 2025-3-25 17:56:49
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Outmoded
发表于 2025-3-25 23:58:57
https://doi.org/10.1007/978-1-4612-4482-0vironments, how do individual stars form and gain mass? Can a forming star cluster be treated as an equilibrium system or is this process too rapid for equilibrium to be established? How does feedback affect the formation process?
描述
发表于 2025-3-26 04:02:26
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cauda-equina
发表于 2025-3-26 04:20:27
The Birth of Massive Stars and Star Clustersvironments, how do individual stars form and gain mass? Can a forming star cluster be treated as an equilibrium system or is this process too rapid for equilibrium to be established? How does feedback affect the formation process?
积习已深
发表于 2025-3-26 10:46:09
Infrared Study of the Southern Galactic Star Forming Region Associated with Iras 10049-5657ased on the MSX data (8, 12, 14, & 21 μm bands). Radiative transfer modelling has been carried out taking into account all available infrared measurements to obtain various physical parameters like nature of the exciting source, geometrical dimensions, dust distribution and composition etc.
QUAIL
发表于 2025-3-26 14:36:06
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Mnemonics
发表于 2025-3-26 17:28:15
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