Distribution of HCO(+) (J = 3-2) in the inner 5 PC of the Galaxy

Details Distribution of HCO(+) (J = 3-2) in the inner 5 PC of the Galaxy Distribution of HCO(+) (J = 3-2) in the inner 5 PC of the Galaxy

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...152l..25s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 152, no. 2, Nov. 1985, p. L25-L28. Research supported by the Naturvetenskaplig

Astronomy and Astrophysics

Astronomy

12

Formyl Ions, Galactic Nuclei, Interstellar Matter, Milky Way Galaxy, Black Holes (Astronomy), Cosmic Dust, Galactic Structure, Molecular Clouds

Scientific paper

Emission from HCO(+) in the 26B-GHz J = 3-2 transition was detected from the IR dust torus surrounding Sgr A (West) in the inner 5 pc of the Galaxy. The distribution of HCO(+) was mapped over a 1.5 x 2 arcmin region with a resolution of 28 arcsec and a grid spacing of 14 arcsec. An analysis of the results reveals a new molecular feature, called the southeast arm, which stretches from the southernmost tip of the south arm of the Sgr A (West) thermal emission toward the north arm and the NE IR maximum.

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