Results from the IAR HI Southern Sky Survey. II. The Magellanic Complex.

Details Results from the IAR HI Southern Sky Survey. II. The Magellanic Complex. Results from the IAR HI Southern Sky Survey. II. The Magellanic Complex.

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998larm.confe..88b&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

Scientific paper

One of the important results of the IAR HI Southern Sky Survey (HISSS) is the mapping of the HI connected to each of the components of the Magellanic Complex, i.e., the Clouds themselves, the Bridge, the Halo and the Magellanic Stream (MS). The obtained maps allow us to study the distribution, velocity field and velocity dispersion of the gas in the mentioned features in order to derive conclusions about their extension, kinematics and dynamics. The main advantages of the use of this Survey for these purposes are based on its large scale coverage and on its uniform high velocity resolution (1 km/s) and high sensitivity (rms=0.07 K).

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