The galactic center at submillimeter and far-infrared wavelengths

Details The galactic center at submillimeter and far-infrared wavelengths The galactic center at submillimeter and far-infrared wavelengths

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..127g&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 127-134 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astronomy

Far Infrared Radiation, Galactic Nuclei, Galactic Structure, Spectrum Analysis, Stellar Spectra, Submillimeter Waves, Galactic Radiation, Interstellar Matter, Interstellar Radiation, Molecular Clouds, Radio Astronomy

Scientific paper

Progress in 10 micron and 1 mm observations of the central 100 pct. of our galaxy and their interpretation is discussed. Emphasis is placed on the physical conditions and dynamics in the nucleus derived from spectroscopic and broadband observations of interstellar gas and dust. The observations suggest that sporadic mass inflow into the central parsec from systems of large, massive molecular clouds dominates the dynamics of the interstellar gas at the Galactic Center. Outflow fits most of the velocity measurements but is much less acceptable than inflow in the overall physical picture now developing.

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