Neutral hydrogen emission-absorption in the IRR II galaxy NGC 5363

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Absorption Spectra, Emission Spectra, Extragalactic Radio Sources, Hydrogen Clouds, Neutral Gases, Cosmic Dust, Galactic Rotation, Galactic Structure, Peculiar Galaxies, Spiral Galaxies

Scientific paper

The neutral hydrogen profile of the peculiar galaxy NGC 5363 reveals broad weak emission characteristic of disk emission from an early-type galaxy, as well as absorption attributed to a cloud located in front of the core continuum source. The peak optical depth of the absorption feature is tau not greater than about 0.06 + or - 0.005. The relatively broad absorption range and its asymmetry likens the feature to those seen in several other systems, in particular that of NGC 253.

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