exhibit 发表于 2025-3-30 11:58:46

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Blood-Clot 发表于 2025-3-30 16:15:56

The Observational Evidence for an Intercloud Mediummedium in the solar neighbourhood has a temperature between 10. and 10. K, a column density of ~1.4×10. cosec |.| atoms cm., and a brightness temperature of ~4.4 cosec |.| K wherever the line of sight does not intersect optically thick cold concentrations.

Carminative 发表于 2025-3-30 18:06:12

Properties of Neutral Hydrogen Clouds/or irregular in shape. Histograms of cloud parameters are presented and subjected to statistical analysis. There is evidence for tenuous clouds of large angular extent but very low column density (.. < 10. cm.).

使成波状 发表于 2025-3-30 20:58:28

Free Electrons Outside H , Regions interarm region. The . thickness of the electron layer in the solar neighbourhood is found to be larger than or of the order of 0.8 kpc. No reliable figure of the electron distribution can be deduced for the moment in the inner parts of the Galaxy.

同音 发表于 2025-3-31 00:51:37

Line Absorption Studies of the Interstellar Gas Near 1015 Hzed in detail using this instrument. A more comprehensive picture may now be developed for element depletion factors, electron densities, and sources of ionization (UV photons, low energy cosmic and .-rays).

macular-edema 发表于 2025-3-31 06:41:31

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极少 发表于 2025-3-31 10:55:28

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Fibroid 发表于 2025-3-31 13:54:04

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EXALT 发表于 2025-3-31 21:06:39

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Console 发表于 2025-3-31 21:43:08

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查看完整版本: Titlebook: Galactic Radio Astronomy; F. J. Kerr,S. C. Simonson Book 1974 International Astronomical Union 1974 Galaxy.astronomy.interstellar matter.p