Multi-Wavelength Surveys of Galactic Star Forming Regions

Details Multi-Wavelength Surveys of Galactic Star Forming Regions Multi-Wavelength Surveys of Galactic Star Forming Regions

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..317...97s&link_type=abstract

Milky Way Surveys: The Structure and Evolution of our Galaxy, Proceedings of ASP Conference #317. The 5th Boston University Ast

Astronomy and Astrophysics

Astrophysics

Scientific paper

The availability of large scale, high angular resolution Galactic continuum surveys from cm to near-IR wave lengths makes complementary spectroscopic surveys increasingly more important. The velocity information provided by spectral line surveys is crucial not only for the study of internal cloud dynamics, but also to determine distances, masses, sizes, and to disentangle clouds along the line of sight in crowded regions and the inner Galaxy.

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