Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...102..134h&link_type=abstract
Astronomy and Astrophysics, vol. 102, no. 1, Sept. 1981, p. 134-141. Deutsche Forschungsgemeinschaft
Astronomy and Astrophysics
Astronomy
95
Astronomical Maps, Galaxies, Hydrogen Clouds, Interstellar Gas, Mass Distribution, Neutral Gases, Intergalactic Media, Magellanic Clouds, Radio Astronomy, Radio Telescopes, Velocity Distribution
Scientific paper
Twenty-one relatively large irregular galaxies spread over an absolute magnitude range between -18.9 and -13.7 are mapped with the 100 m radio telescope at Effelsberg at a wavelength of 21 cm to derive global parameters, to search for extended H I envelopes, and to study the influence of the envelope on the integrated profile. A model-fit-technique is used to determine the parameters of the H I distribution, the geometry, and the rotation of the galaxies for objects smaller than 20 arcmin in angular extent. The half power width of the observed H I distribution is similar to the Holmberg diameters, and eight of the galaxies have extended H I envelopes at a low H I surface density of 10 to the 19th atoms per sq cm.
Huchtmeier Walter K.
Materne J.
Seiradakis John H.
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