Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Oct-2021)

Result of query: info cati KIC$
 -Dec-2012 - Modification
Details on Acronym:   KELT
   KELT Write:<<KELT -NN>>
<<KELT -NNA>>
<<KELT -NNa>>
<<KELT -NNAa>> Originof the Acronym: p = Pre-registered to IAU Comm.5 ar clusters in M 31: 2 new clusters are found, which are not in Bol nor SKHB. in source:M 31 = NGC 224 Ref:=1989AJ.....98.2080K byKENT S.M. , HUCHRA J.P., STAUFFER J. Astron. J., 98, 2080-2085 (1989) The shape of the mass distribution in M 31 from its globular cluster system. oTable III: <[KHS89] BHHMMSS.s+DDMMSS> N=2.
Details on Acronym:   [KHT2016]
   [KHT2016] (Kounkel+Hartmann+Tobin+, 2016) Write:<<[KHT2016] ONC RVNNNN>>
<<[KHT2016] NGC2264 RVNNNN>> N: 1154+903 Object:*  (SIMBAD class: Star) Note:Magellan/M2FS, MMT Hectospec and Magellan Clay MIKE spectroscopy of N=1154+903 stars of the two closest massive star-forming regions, ONC and NGC 2264. in source:NGC 2264 in source:NAME ONC Ref:=2016ApJ...821....8K byKOUNKEL M. , HARTMANN L., TOBIN J.J., MATEO M., BAILEY III J.I., SPENCER M. Astrophys. J., 821, 8-8 (2016) Spectroscopic binaries in the Orion nebula cluster and NGC 2264. oTable 2: <[KHT2016] ONC RVNNNN> (Nos 1-1154), <[KHT2016] NGC2264 RVNNNN> (Nos 1155-2057). =E=Catalogue in electronic form as J/ApJ/821/8 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [KHU96]
   [KHU96] (Koyama+Hamaguchi+Ueno+, 1996) Write:<<[KHU96] N>> N: 8 Object:(X )  (SIMBAD class: X = X-ray source) Stat:is completely incorporated in Simbad Note:ASCA satellite observations in source:NAME R CrA Cloud Ref:=1996PASJ...48L..87K byKOYAMA K. , HAMAGUCHI K., UENO S., KOBAYASHI N., FEIGELSON E.D. Publ. Astron. Soc. Jap., 48, 87-92 (1996) Discovery of hard X-rays from a cluster of protostars. oTable 1: <[KHU96] N> (Nos 1-8). <NAME CORONET CLUSTER> Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [KHV2011]
   [KHV2011] (Kuiper+Hatch+Venemans+, 2011)

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