A 21 CM hydrogen line survey of the Small Magellanic Cloud

Details A 21 CM hydrogen line survey of the Small Magellanic Cloud A 21 CM hydrogen line survey of the Small Magellanic Cloud

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...48...71b&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 48, Apr. 1982, p. 71-80.

Astronomy and Astrophysics

Astrophysics

18

Astronomical Maps, Astronomical Spectroscopy, Centimeter Waves, H Lines, Magellanic Clouds, Spectral Line Width, Contours, Galactic Rotation, High Resolution, Hydrogen Atoms, Radio Telescopes

Scientific paper

Contour maps are presented for a complete, 21-cm HI line survey of the Small Magellanic Cloud, conducted in the alpha 0 to 30 deg, delta -76 to -70 deg region with the IAR 30-m dish. While good agreement is found between the present maps and those of Hindman and Balnaves (1967), improvements have been achieved in velocity resolution, permitting the determination of a better rotation curve, and in the separation of different components along the line of sight. Attention is given the HI features of the eastern zone.

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