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 |
| by | YUSEF-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. | |
| o | p.668, 4.: binary system CX 5 = [PPL2002] CX 5. |
| o | Fig.2: <[YLW2002] AN> (Nos A1-A5). |
| Ref: | =2004ApJ...611..858L |
| by | LAW C. , YUSEF-ZADEH F. |
| Astrophys. J., 611, 858-870 (2004) | |
| X-ray observations of stellar clusters near the galactic center. | |
| o | Table 1: candidate clusters DB00 and DB01 are respectively [DB2000] NN and [DB2001] Cl NN in SIMBAD. |
| o | Fig.1, Table 2: <[YLW2002] ANW> (Nos A1N, A1S) added. Fig.2, Table 2: <[LY2004] QXN> (Nos QX1-QX4). |
| Ref: | =2006MNRAS.371...38W |
| by | WANG 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. | |
| o | Table 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 |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |