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

Watemelon

BRIBE

催眠藥

New High Spectral Resolution Airborne Line Observations in the Far Infrareds been detected in the Orion Nebula. The intensity of this line is discussed compared with theoretical predictions. Preliminary results concerning the observations of OIII (88μ) in the Orion Nebula are also presented.

Fresco

Asymptomatic

Balloon Observation of the Milky Way at Wavelength 2.4 μmghtness temperature of radio continuum and shows humps at the same positions as was found for the intensity of 2.6 mm line of CO. This suggests the contribution of young objects to the infrared brightness. The isophotes of the infrared intensity are compared with that expected for models of the galaxy.

詞匯表

祖?zhèn)髫?cái)產(chǎn)

殺人

疏遠(yuǎn)天際

discord

High-Energy Gamma-Ray Results from the COS-B Satellite and Infrared Astronomyof the preliminary results indicate that a fraction of the galactic gamma-rays originate in close-by regions (distance ≤ 1 kpc). The interpretation of these results in correlation with infrared observations will permit a study of the content structure of the local interstellar medium.