Dictionary of Nomenclature of Celestial Objects
(Last update: 08-Oct-2020)

Result of query: info cati CBW2017] GLLL.llll+BB.bbbb-MMN$



.
 

Details on Acronym:   [CBW2017]
   [CBW2017] (Csengeri+Bontemps+Wyrowski+, 2017) Write:<<[CBW2017] GLLL.llll+BB.bbbb-MMN>>
<<[CBW2017] LLL.llll+B.bbbb-MMN>> (not recognised by Simbad, but found in literature) N: 100 Object:Clump  (SIMBAD class: Radio(sub-mm) = sub-millimetric source) Note:ALMA Band 7 Cycle 2 observations of N=100 sources in 35 infrared-quiet massive clumps selected from the ATLASGAL survey. Ref:=2017A&A...600L..10C byCSENGERI T. , BONTEMPS S., WYROWSKI F., MOTTE F., MENTEN K.M., BEUTHER H., BRONFMAN L., COMMERCON B., CHAPILLON E., DUARTE-CABRAL A., FULLER G.A., HENNING T., LEURINI S., LONGMORE S., PALAU A., PERETTO N., SCHULLER F., TAN J.C., TESTI L., TRAFICANTE A., URQUHART J.S. Astron. Astrophys., 600L, 10-10 (2017) ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumps. oFig. A.1, Table A.1: <[CBW2017] GLLL.llll+BB.bbbb-MMN> N=100. =E=Catalogue in electronic form as <J/A+A/600/L10/> Originof the Acronym: S = Created by Simbad, the CDS Database

© Université de Strasbourg/CNRS

    • Contact