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A Large-Scale CO Imaging of the Galactic Center
Published online by Cambridge University Press: 25 May 2016
Extract
Molecular gas in the Galactic center region is spatially and kinematically complex, and its physical conditions are distinctively different from those of molecular gas in the Galactic disk (e.g., Morris 1996). Relative paucity of current star formation activity, despite the abundance of dense molecular gas in this region, is one of the problem at issue.
- Type
- Part 3. The Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 189 - 190
- Copyright
- Copyright © Kluwer 1998