Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati RRA2004] HH 108 VLA N$
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Details on Acronym:   [RRA2004]
  
[RRA2004] (Reipurth+Rodriguez+Anglada+, 2004)= (VLA)
Write:<<[RRA2004] Haro 6-10 VLA NA>>
<<[RRA2004] NGC 2023 MM VLA N>>
<<[RRA2004] NGC 2264 MM VLA N>>
<<[RRA2004] HH 108 VLA N>>
<<[RRA2004] JHHMMSSs+DDMMSS>>
N: 3+3+8+2+1
Object:(Rad)  (SIMBAD class: Radio = Radio Source)
Stat:is completely incorporated in Simbad
Note:VLA observations of young outflow sources. The driving source of the outflow in NGC 2264 is identified by its coordinates.
in source:Haro 6-10
in source:NGC 2023
in source:NGC 2264
in source:HH 108
Ref:=2004AJ....127.1736R
byREIPURTH B. , RODRIGUEZ L.F., ANGLADA G., BALLY J.
 Astron. J., 127, 1736-1746 (2004)
  Radio continuum jets from protostellar objects.
oTable 2: <[RRA2004] Haro 6-10 VLA NA> (Nos 1-3, 1B), <[RRA2004] NGC 2023 MM VLA N> (Nos 1-3), <[RRA2004] NGC 2264 MM VLA N> (Nos 1-8), <[RRA2004] HH 108 VLA N> (Nos 1-2). Text: <[RRA2004] JHHMMSSs+DDMMSS> N=1. Table 2: <[RRC99] VLA NN> (Nos 15-18) added. Table 2: <[RR96] HH 199 N> (Nos 3-4) added. Table 2: <[BEA2001] L1251A NN> (Nos 10-11) added.
Originof the Acronym: S = Created by Simbad, the CDS Database

Details on Acronym:   VLA
  
VLA (Very Large Array)
***** Avoid the usage of VLA, prefer [RRA2004]
Originof the Acronym: A = Assigned by the author(s)