HI Study of Barred Magellanic Type Galaxies

Details HI Study of Barred Magellanic Type Galaxies HI Study of Barred Magellanic Type Galaxies

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...18510505w&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #105.05; Bulletin of the American Astronomical Society, Vol. 26, p.1492

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Scientific paper

We present the preliminary results of an HI survey of a small sample of Barred Magellanic type galaxies. The data were obtained using the D configuration of the VLA and our observations show: (1) bar morphology seen in the optical data is manifested in the HI distribution and kinematics, (2) SBm/IBm galaxies are commonly found with gaseous companions, and (3) there is strong evidence of significant gravitational interaction between the SBm/IBm galaxy and its companion. These data complement other study in suggesting that gravitational interactions play a strong role in determining the physical properties of SBm/IBm galaxies.

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