Titlebook: Infrared and Submillimeter Astronomy; Proceedings of a Sym Giovanni G. Fazio Conference proceedings 1977 D. Reidel Publishing Company, Dord

知識(shí)

Long-Term Infrared Monitoring of Stellar Sources from Earth Orbits of circumstellar microwave line emission that may be pumped by the variable infrared continuum near the wavelength of observation. Strong coupling of large-scale convection and pulsation can give rise to the circumstellar clouds and, under certain conditions, may even provide the mechanism for eje

MEEK

機(jī)警

Lipoprotein

High Resolution Mapping of the Orion Nebula Region at 30, 50 and 100 Micronsed by a central luminosity source. D) At all three wavelengths, the surface brightness of the emission in the direction of the H II region is measured to be less than 10% of the peak surface brightness. The color temperature of this emission is ≤ 200 K. E) At 50 μ and 100 μ, there is a strong sugges

燕麥

敲竹杠

凹槽

Prediction of the Diffuse Far-Infrared Flux from the Galactic Plane0° and the far-infrared emissivity as a function of galactocentric distance. Future measurements of the galactic far-infrared flux would yield valuable information on the physical properties and distribution of dust and molecular clouds in the galaxy, particularly the inner region.

ECG769

NUL

ligature