.
Details on Acronym: CG-NGP
CG-NGP (Corbally+Garrison, North Gal. Pole) ***** Avoid the usage of CG-NGP, prefer CGG* NGP Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: CGG* NGP
CGG* NGP (Corbally+Garrison, G *, North Gal. Pole)= (CG-NGP) Write:<<CGG* NGP NNN>> N: 192 Object:Dw. * (SIMBAD class: Star) Note:The authors use the designation 'CG-NGP', which can't be used in SIMBAD Plates See also CGG* SGP in source:NAME NGP Ref:=1988AJ.....95..745C byCORBALLY C.J. , GARRISON R.F. Astron. J., 95, 745-749 (1988) A search for early-G dwarf stars the North Galactic Pole. oTable II: <CG-NGP NNN> use <CGG* NGP NNN>, (Nos 1-192) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: NGP
NGP (North Gal. Pole) ***** Avoid the usage of NGP, prefer FAUST Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: NGP
NGP (North Gal. Pole)= (UL) = (Up) = (Upgren) Write:<<NGP DD NNN>> N: 4027 Object:Late * (SIMBAD class: Star) Note:Somtimes found with the format 'DD-NNN'. declinaison zones: 25 to 50. Identif. charts (no coordinates). in source:NAME NGP Ref:=1962AJ.....67...37U byUPGREN A.R. Astron. J., 67, 37-78 (1962) The space distribution of late type stars in a North Galactic Pole region. oCatalogue: <NGP DD NNN> N=4027 =E=Catalogue in electronic form as III/10 =E=Catalogue in electronic form as <III/10B/> Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: NGP
NGP (North Gal. Pole) ***** Avoid the usage of NGP, prefer SNGP Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: NGP
NGP (North Gal. Pole) ***** Avoid the usage of NGP, prefer Ton
Details on Acronym: NGP
NGP (North Gal. Pole) ***** Avoid the usage of NGP, prefer [YDM2001] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: UL
UL (Upgren, Late spectral type) ***** Avoid the usage of UL, prefer NGP
Details on Acronym: Up
Up (Upgren) ***** Avoid the usage of Up, prefer NGP
Details on Acronym: Upgren
Upgren (Upgren) ***** Avoid the usage of Upgren, prefer NGP
© Université de Strasbourg/CNRS
• Contact