Dictionary of Nomenclature of Celestial Objects (Last update: 24-Jan-2023)
Result of query: info cati YLW2002] AN$
Details on Acronym: [YLW2002] [YLW2002] (Yusef-Zadeh+Law+Wardle+, 2002)
Object:(X) (SIMBAD class: X = X-ray Source)
Stat:is completely incorporated in SimbadNote:Chandra observations of the Arches Cluster: N=5 components (Nos A1-A6). Component A1 is a double source.
in source:NAME Arches ClusterRef:=2002ApJ...570..665Y
, 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).
, 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).
, 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/371/38Originof the Acronym: S = Created by Simbad, the CDS Database