Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Sep-2023)

Result of query: info cati YLW2002] AN$


Details on Acronym:   [YLW2002]
   [YLW2002] (Yusef-Zadeh+Law+Wardle+, 2002) Write:<<[YLW2002] ANW>> N: 6+2 Object:(X)  (SIMBAD class: X = X-ray Source) Stat:is completely incorporated in Simbad Note:Chandra observations of the Arches Cluster: N=5 components (Nos A1-A6). Component A1 is a double source. in source:NAME Arches Cluster Ref:=2002ApJ...570..665Y byYUSEF-ZADEH F. , LAW C., WARDLE M., WANG Q.D., FRUSCIONE A., LANG C.C., COTERA A. Astrophys. J., 570, 665-670 (2002) Detection of X-ray emission from the Arches cluster near the Galactic Center. op.668, 4.: binary system CX 5 = [PPL2002] CX 5. oFig.2: <[YLW2002] AN> (Nos A1-A5). Ref:=2004ApJ...611..858L byLAW C. , YUSEF-ZADEH F. Astrophys. J., 611, 858-870 (2004) X-ray observations of stellar clusters near the galactic center. oTable 1: candidate clusters DB00 and DB01 are respectively [DB2000] NN and [DB2001] Cl NN in SIMBAD. oFig.1, Table 2: <[YLW2002] ANW> (Nos A1N, A1S) added. Fig.2, Table 2: <[LY2004] QXN> (Nos QX1-QX4). Ref:=2006MNRAS.371...38W byWANG Q.D. , DONG H., LANG C. Mon. Not. R. Astron. Soc., 371, 38-54 (2006) The interplay between star formation and the nuclear environment of our Galaxy: deep X-ray observations of the Galactic centre Arches and Quintuplet clusters. oTable 1, col(1): <[WDL2006] NNN> (Nos 1-244) = Table 1, col(2): <CXOGCS JHHMMSS.ss+DDMMSS.s> N=244. Fig.2, Table 2: <[YLW2002] AN> (No. A6) added, <[LY2004] QXN> (No. QX5) added. =E=Catalogue in electronic form as J/MNRAS/371/38 Originof the Acronym: S = Created by Simbad, the CDS Database

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