Titlebook: CO: Twenty-Five Years of Millimeter-Wave Spectroscopy; Proceedings of the 1 William B. Latter,Simon J. E. Radford,John Bally Conference pro

Mosaic

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

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

安慰

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

傳染

喪失

GONG

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