向下
发表于 2025-3-26 22:04:07
The Ursa Major Molecular Cloudsentered at (.) ∼ (138°,30°) and easily seen in IRAS 100 μm emission, is some 60 pc across and 150 pc distant (Meyerdierks et. al 1991). At 100 μm, the Ursa Major clouds appear in projection as “finger” (. ∼ 140,. ∼; 38) which “hangs down” towards the center of the loop and the plane of the Galaxy. D
GUILE
发表于 2025-3-27 02:47:45
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珍奇
发表于 2025-3-27 05:27:42
The CO 2-1/1-0 Ratio solar neighborhood exhibit variations of the .=2−1/ .=l−0 intensity ratio from place to place in a cloud and from one cloud to another. This mainly reflects a variation of the hydrogen density near the ., where the opacity of the lines reaches ∼ 1 at cloud surfaces. The ratio often exceeds unity at
曲解
发表于 2025-3-27 10:44:47
http://reply.papertrans.cn/23/2205/220410/220410_34.png
Project
发表于 2025-3-27 16:37:25
On the Fractal Structure of Molecular Cloudsects of star formation. Being generated predominantly by the turbulent internal cloud motion, the structure of molecular clouds is likely to be random to a large degree. As the information on the structural properties of random function is basically contained in its power spectrum, it is obviously i
grandiose
发表于 2025-3-27 21:21:43
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亲密
发表于 2025-3-28 00:40:03
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偏离
发表于 2025-3-28 05:23:22
http://reply.papertrans.cn/23/2205/220410/220410_38.png
冷峻
发表于 2025-3-28 07:17:00
Narratives of Hurricane Katrina in Contextes easier to understand the evolution of the disk of stars. The star formation rate per unit molecular gas mass is constant as a function of radius, and the H. depletion time turns out to be only a few percent of the Hubble time. This very short timescale requires that the atomic gas act as a reserv
破译密码
发表于 2025-3-28 14:02:36
https://doi.org/10.1007/978-3-319-59957-1a sensitivity per solid angle 3-10 times higher than previous CO surveys of the plane, and 16 times higher than the only previous extensive wide-latitude survey (Dame et al. 1987). Since a preliminary purpose of this survey is the study of molecular gas out of the plane in the inner Galaxy, the obse