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

Result of query: info cati GZK2010] MMN-Main$
.

Details on Acronym:   [GZK2010]
  
[GZK2010] (Galvan-Madrid+Zhang+Keto+, 2010)
Write:<<[GZK2010] MMN-Main>>
<<[GZK2010] MMN-WW>>
<<[GZK2010] MM1-Ridge>>
N: 2+5+1
Object:(mm)  (SIMBAD class: mmRad = Millimetric Radio Source)
Note:2010ApJ...725...17G: SMA 1.3mm and 0.9mm continuum observations of N=5 sources in the W33A massive star formation region.
2017MNRAS.467L.120M: ALMA band 6 (230GHz) and 7 (345GHz) observations of N=3 sources in [VVE2000] W33A MM 1.
in source:W 33:W 33A = W 33A
Ref:=2010ApJ...725...17G
byGALVAN-MADRID R. , ZHANG Q., KETO E., HO P.T.P., ZAPATA L.A., RODRIGUEZ L.F., PINEDA J.E., VAZQUEZ-SEMADENI E.
 Astrophys. J., 725, 17-28 (2010)
  From the convergence of filaments to disk-outflow accretion: massive star formation in W33A.
oTable 2: <[GZK2010] MMN-Main> (Nos MM1-Main and MM2-Main), <[GZK2010] MMN-WW> (Nos MM1-NW, MM1-SE, MM2-NE).
Ref:=2017MNRAS.467L.120M
byMAUD L.T. , HOARE M.G., GALVAN-MADRID R., ZHANG Q., DE WIT W.J., KETO E., JOHNSTON K.G., PINEDA J.E.
 Mon. Not. R. Astron. Soc., 467L, 120-124 (2017)
  The ALMA view of W33A: a spiral filament feeding the candidate disc in MM1-Main.
oFig. 1, Table 1: <[GZK2010] MM1-W> (Nos E, S) added, <[GZK2010] MM1-Ridge> N=1.
Originof the Acronym: S = Created by Simbad, the CDS Database