Dictionary of Nomenclature of Celestial Objects

Small-scale structure of [MSM77] MS V and VI in the Magellanic Stream.
N=3 HI small clumps in MS V, and N=4 HI small clumps in MS VI. N=2 large clumps in MS V and MS VI, in MS V the large clump has two components H and L for the Higher and the Lower component velocity.
Other structures are described in the text. See also [MSM77], [MCD79]. in source:Magellanic Clouds:Magellanic Stream = Magellanic Stream Ref:=2002ApJ...576..773S bySTANIMIROVIC S. , DICKEY J.M., KRCO M., BROOKS A.M. Astrophys. J., 576, 773-789 (2002) The small-scale structure of the Magellanic stream. oTable 1: <[SDK2002] MS V N> (Nos 1-3), <[SDK2002] MS VI N> (Nos 1-4), <[SDK2002] MS V A> (Nos H, L), <[SDK2002] MS VI> N=1. Text p.776: <[SDK2002] MS VI looplike> N=1, <[SDK2002] MS V round cloud> N=1, <[SDK2002] MS V straight filament> N=1, <[SDK2002] MS V curved filament> N=1.
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