OFF 发表于 2025-3-30 08:12:57
http://reply.papertrans.cn/39/3804/380338/380338_51.png安心地散步 发表于 2025-3-30 13:25:04
http://reply.papertrans.cn/39/3804/380338/380338_52.png仔细阅读 发表于 2025-3-30 17:27:59
http://reply.papertrans.cn/39/3804/380338/380338_53.pngPituitary-Gland 发表于 2025-3-31 00:23:15
Molecules as Probes of the Interstellar Medium and of Star Formation,was restricted to use of the 21-cm line of HI and to optical absorption lines of several atoms (Na, Ca, Fe, K, Ti) toward nearby hot stars. To avoid excessive extinction, the optical techniques were limited both to distances of < 1 kpc from the Sun and to diffuse clouds (visual extinction < 2 magn).希望 发表于 2025-3-31 01:40:24
http://reply.papertrans.cn/39/3804/380338/380338_55.png拔出 发表于 2025-3-31 06:59:12
Astronomical Masers,iding a fascinating astrophysical laboratory for the study of maser processes, the intense emissions have been used as probes of the dynamics and physical conditions of their surroundings on scales as small as one astronomical unit throughout the Galaxy and in nearby galaxies. Since masers are found无聊的人 发表于 2025-3-31 09:33:28
The Structure of Our Galaxy Derived from Observations of Neutral Hydrogen,rticularly suitable. Neutral atomic hydrogen, HI, is the main observed constituent of the interstellar medium; its physical properties are closely related to the properties of other Galactic constituents, both stellar and interstellar. The interstellar medium is transparent enough to hydrogen emissi学术讨论会 发表于 2025-3-31 16:19:25
http://reply.papertrans.cn/39/3804/380338/380338_58.png