Mosaic
发表于 2025-3-28 14:59:33
https://doi.org/10.1007/978-3-319-59957-1ry to study diffuse γ-ray emission from the interstellar medium (ISM). High-energy γ rays produced in cosmic-ray (CR) interactions in the ISM can be used to determine the CR density and calibrate the CO line as a tracer of molecular mass. Dominant production mechanisms for γ rays of energies ∼30 MeV
dendrites
发表于 2025-3-28 20:18:38
Springer Series in Transitional Justiceinterstellar medium. The trace ionization within the molecular gas is governed primarily by UV photoionization. Magnetic fields contribute a significantly larger fraction of the pressure in molecular clouds than in the diffuse interstellar medium. Observations suggest that the total Alfvén Mach numb
reception
发表于 2025-3-29 02:43:40
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安慰
发表于 2025-3-29 03:19:08
Dubravka Zarkov,Marlies Glasiusponent of the interstellar medium and to determine the relationship of this component to spiral arm features. When completed in Spring 1996, the CO Survey will cover 103° < .. < 145°, -3° < .. < 5°, and −150 < V. < 50 km s. with angular sampling of 50″ and velocity resolution of 0.8 km s. . During t
传染
发表于 2025-3-29 07:25:24
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丧失
发表于 2025-3-29 15:22:49
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GONG
发表于 2025-3-29 19:01:00
https://doi.org/10.1007/978-3-031-07773-9ects 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