Location of the thermal continuum source Sagittarius D

Details Location of the thermal continuum source Sagittarius D Location of the thermal continuum source Sagittarius D

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...379l..53l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 379, Oct. 1, 1991, p. L53-L56.

Astronomy and Astrophysics

Astronomy

13

Continuous Radiation, Forbidden Bands, Molecular Clouds, Sagittarius Constellation, Thermal Emission, Extragalactic Radio Sources, Galactic Nuclei, Infrared Sources (Astronomy), Milky Way Galaxy, Star Formation

Scientific paper

Very peculiar kinematics of the dense molecular gas in the inner 500 pc of the Milky Way are discussed on the basis of observations of the CS J = 5-4 and CO J = 3-2 emission toward the Sgr D continuum source. The distribution of the CS emission correlates well with the millimeter and radio continuum emission, which suggests that these tracers all originate in the same region. The central velocity of the CS line is consistent with that of the H91-alpha radio recombination line, which indicates that the H II region is associated with the core.

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