Published reference:
An HI Rogues Gallery,
Hibbard, J.E.,
van
Gorkom, J.H.,
Rupen, M.P.,
& Schiminovich,
D.S., 2001, in
ASP Conf. Ser. 240, Gas & Galaxy Evolution, eds.
J.E. Hibbard, M.P. Rupen, & J.H. van Gorkom, (ASP, San Francisco), 659
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- ...interaction
-
This is a somewhat circular argument,
since the prime evidence for an interaction is often the extent of the gas
distribution, and there are papers in the literature for nearly all of
the objects in this class claiming an interacting or merging origin
based on this fact.
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- ...Clouds
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We note that many of the galaxies
in other parts of the Gallery have HI clouds with no identified
optical counterparts, but are classified according to their most
dominant HI characteristics.
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John Hibbard
Tue Sep 18 17:11:04 EDT 2001