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

Result of query: info cati YLW2002] AN$

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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