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

Result of query: info cati MMM2008] N171 N$
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Details on Acronym:   [MMM2008]
  
[MMM2008] (Minamidani+Mizuno+Mizuno+, 2008)
Write:<<[MMM2008] 30 Dor N>>
<<[MMM2008] NNNN NN>>
<<[MMM2008] N206D N>>
<<[MMM2008] GMC 225 N>>
N: 5+10+6+5+2+1+3
Object:CO Clump  (SIMBAD class: MolCld = Molecular Cloud)
Stat:is completely incorporated in Simbad
Note:ASTE, Mopra, and SEST CO line observations of giant molecular clouds in the LMC.
in source:Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
in source:Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
in source:Magellanic Clouds:LMC:LHA 120-N 171 = LHA 120-N 171
in source:Magellanic Clouds:LMC:LHA 120-N 166 = LHA 120-N 166
in source:Magellanic Clouds:LMC:LHA 120-N 206 = LHA 120-N 206
Ref:=2008ApJS..175..485M
byMINAMIDANI T. , MIZUNO N., MIZUNO Y., KAWAMURA A., ONISHI T., HASEGAWA T., TATEMATSU K., IKEDA M., MORIGUCHI Y., YAMAGUCHI N., OTT J., WONG T., MULLER E., PINEDA J.L., HUGHES A., STAVELEY-SMITH L., KLEIN U., MIZUNO A., NIKOLIC S., BOOTH R.S., HEIKKILAE A., NYMAN L.-A., LERNER M., GARAY G., KIM S., FUJISHITA M., KAWASE T., RUBIO M., FUKUI Y.
 Astrophys. J., Suppl. Ser., 175, 485-508 (2008)
  Submillimeter observations of giant molecular clouds in the Large Magellanic Cloud: temperature and density as determined from J=3-2 and J=1-0 transitions of CO.
oTable 2: <[MMM2008] 30 Dor N> (Nos 1-5), <[MMM2008] N159 NN> (Nos 1-10), <[MMM2008] N171 N> (Nos 1-6), <[MMM2008] N166 N> (Nos 1-5), <[MMM2008] N206 N> (Nos 1-2), <[MMM2008] N206D N> (No. 1), <[MMM2008] GMC 225 N> (Nos 1-3).
Originof the Acronym: S = Created by Simbad, the CDS Database