Aperture-synthesis observations of H I in the galaxy NGC 300

Details Aperture-synthesis observations of H I in the galaxy NGC 300 Aperture-synthesis observations of H I in the galaxy NGC 300

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...229..509r&link_type=abstract

Astrophysical Journal, Part 1, vol. 229, Apr. 15, 1979, p. 509-513.

Astronomy and Astrophysics

Astronomy

40

H Lines, Hydrogen Clouds, Interferometry, Radio Sources (Astronomy), Spiral Galaxies, Brightness Temperature, Centimeter Waves, Galactic Structure, Velocity Distribution

Scientific paper

A high-resolution aperture-synthesis study of the spiral galaxy NGC 300 has been carried out in the H I line. A peculiar velocity field outside the optical image of the galaxy was found and is interpreted as being due to a substantial warping of the outer plane of the galaxy. This distortion may be related to the presence of massive H I companions to NGC 300. The more normal H I properties of NGC 300 are also discussed.

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