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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)
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