Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...385..188b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 385, Jan. 20, 1992, p. 188-192.
Astronomy and Astrophysics
Astronomy
12
Formaldehyde, Galactic Nuclei, Interstellar Matter, Molecular Absorption, Radio Sources (Astronomy), Carbon Monoxide, Hydrogen, Rotating Disks, Velocity Distribution
Scientific paper
NGC 3628 displays strong absorption against the extended nuclear radio source. Results from a VLA study of the nuclear H2CO absorption and Arecibo H I data are reported here and are integrated with those from earlier H I and OH emission and absorption studies. The nuclear absorption originates in two components: a rapidly rotating molecular disk and an anomalous structure with a distinctly different velocity gradient and central velocity. The anomalous structure is interpreted in terms of the perturbed density and velocity field, resulting from a recent interaction with NGC 3627, another member of the Leo Triplet.
Baan Willem A.
Goss William Miller
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