On the nature of the hard X-ray source IGR J2018+4043
We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018+4043 in the multiwavelength observations of the source field. The source, originally discovered in the 20-40 keV band, is now confidently detected also in the 40-80 keV band, with a flux of (1.4 ± 0.4) × 10-11...
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| Autores principales: | Bykov, A.M., Krassilchtchikov, A.M., Uvarov, Yu.A., Kennea, J.A., Pavlov, G.G., Dubner, G.M., Giacani, E.B., Bloemen, H., Hermsen, W., Kaastra, J., Lebrun, F., Renaud, M., Terrier, R., Debecker, M., Rauw, G., Swings, J.-P. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n1II_pL21_Bykov |
| Aporte de: |
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