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...
Guardado en:
| Publicado: |
2006
|
|---|---|
| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v649_n1II_pL21_Bykov http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n1II_pL21_Bykov |
| Aporte de: |
Ejemplares similares
-
On the nature of the hard X-ray source IGR J2018+4043
por: Bykov, A.M., et al. -
Isolated X-ray-infrared sources in the region of interaction of the supernova remnant IC 443 with a molecular cloud
Publicado: (2008) -
Isolated X-ray-infrared sources in the region of interaction of the supernova remnant IC 443 with a molecular cloud
por: Bykov, A.M., et al. -
Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
Publicado: (2005) -
Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
por: Warren, J.S., et al.