Details on Acronym: [WC2002] | |
[WC2002] | (Wang+Chakrabarty, 2002) |
Write: | <<[WC2002] XN>> |
N: | 9 |
Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
Stat: | is completely incorporated in Simbad |
Note: | XMM-Newton search for an infrared counterpart of 1E 1048.1-5937. N=9 candidates, (Nos X1-X9), X1 being the proposed counterpart in the first paper and X9 in the second paper. |
Ref: | =2002ApJ...579L..33W |
by | WANG Z. , CHAKRABARTY D. |
Astrophys. J., 579, 33-36 (2002) | |
The likely near-infrared counterpart to the anomalous X-ray pulsar 1E 1048.1-5937. | |
o | Table 1: (Nos A-D) = [MCB92] Star A to D, f = Chandra position of 1E 1048.1-5937. |
o | Table 1: <[WC2002] XN> (Nos X1-X8). |
Ref: | =2002ApJ...580L.143I |
by | ISRAEL G.L. , COVINO S., STELLA L., CAMPANA S., MARCONI G., MEREGHETTI S., MIGNANI R., NEGUERUELA I., OOSTERBROEK T., PARMAR A.N., BURDERI L., ANGELINI L. |
Astrophys. J., 580, 143-146 (2002) | |
The detection of variability from the candidate infrared counterpart to the anomalous X-ray pulsar 1E 1048.1-5937. | |
o | Fig.2: <[WC2002] XN> (No. X9) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |