Dictionary of Nomenclature of Celestial Objects
(Last update: 05-Dec-2023)

Result of query: info cati SDK2002] MS VI N$

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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
     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.
 Originof the Acronym: S = Created by Simbad, the CDS Database