Dictionary of Nomenclature of Celestial Objects
(Last update: 18-Jun-2021)

Result of query: info cati BBG2017]$

Details on Acronym:   [BBG2017]
   [BBG2017] (Bitsakis+Bonfini+Gonzalez-Lopezlira+, 2017) Write:<<[BBG2017] IR1-NNNN>>
<<[BBG2017] M2-NNNN>>
<<[BBG2017] NUV-NNNN>>
<<[BBG2017] IR1_NNNN>> (not recognised by Simbad, but found in literature)
<<[BBG2017] M2_NNNN>>
<<[BBG2017] NUV_NNNN>> N: 2373+741+736 Object:Cluster of *  (SIMBAD class: Cl* = Cluster of Stars) Note:N=4850 star clusters in the Large Magellanic Cloud.
Use of archival data from GALEX, SUMAC survey (Swift/UVOT Magellanic Clouds Survey), MCPS survey (Magellanic Cloud Photometric Survey), and Spitzer SAGE.
See also [BGB2018]. in source:Magellanic Clouds:LMC = LMC Ref:=2017ApJ...845...56B byBITSAKIS T. , BONFINI P., GONZALEZ-LOPEZLIRA R.A., RAMIREZ-SIORDIA V.H., BRUZUAL G., CHARLOT S., MARAVELIAS G., ZARITSKY D. Astrophys. J., 845, 56-56 (2017) A novel method to automatically detect and measure the ages of star clusters in nearby galaxies: application to the Large Magellanic Cloud. oTable 2: <[BBG2017] IR1-NNNN> N=2373 among (Nos IR1-1 to IR1-2653), <[BBG2017] M2-NNNN> N=741 among (Nos M2-3 to M2-1294), <[BBG2017] NUV-NNNN> N=1736 among (Nos NUV-2 to NUV-2334). =E=Catalogue in electronic form as <J/ApJ/845/56/> Originof the Acronym: S = Created by Simbad, the CDS Database

© Université de Strasbourg/CNRS

    • Contact