Details on Acronym: [SDK2002] | |
[SDK2002] | (Stanimirovic+Dickey+Krco+, 2002) |
Write: | <<[SDK2002] MS V N>> <<[SDK2002] MS VI N>> <<[SDK2002] MS V A>> <<[SDK2002] MS VI>> <<[SDK2002] MS VI looplike>> <<[SDK2002] MS V east>> <<[SDK2002] MS V west ridge>> <<[SDK2002] MS V round cloud>> <<[SDK2002] MS V straight filament>> <<[SDK2002] MS V curved filament>> |
N: | 3+4+2+1+1+1+1+1 |
Object: | HI Clump (SIMBAD class: Unknown = Object of Unknown Nature) |
Stat: | is completely incorporated in Simbad |
Note: | Arecibo observations. 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 |
by | STANIMIROVIC S. , DICKEY J.M., KRCO M., BROOKS A.M. |
Astrophys. J., 576, 773-789 (2002) | |
The small-scale structure of the Magellanic stream. | |
o | Table 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. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |