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- W109475049 abstract "Abstract. The availability of large scale, high angular resolution Galac-tic continuum surveys from cm to near-IR wave lengths makes complementaryspectroscopic surveys increasingly more important. The velocity informationprovided by spectral line surveys is crucial not only for the study of internalcloud dynamics, but also to determine distances, masses, sizes, and to disentan-gle clouds along the line of sight in crowded regions and the inner Galaxy. 1. IntroductionDue to advances in array receiver technology and observing techniques, in par-ticular on the fly mapping, spectral line surveys on large to even Galactic scaleshave become feasible. While lower frequency surveys, such as the BU-FCRAO 13 CO J = 1 → 0 Galactic Ring Survey, reveal the bulk of the molecular materialtypically at low densities and temperatures, observations of higher excited linesofCOisotopomersandbothatomiccarbonlinesyieldadditionalimportantcluesto the excitation conditions, the kinematics, the UV field, and the chemistry inparticular of the star formation sites in the clouds.2. Large Scale Study of the Cygnus X RegionCygnus X is a nearby high mass star forming complex with several 10" @default.
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- W109475049 date "2004-12-01" @default.
- W109475049 modified "2023-09-26" @default.
- W109475049 title "Multi-Wavelength Surveys of Galactic Star Forming Regions" @default.
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