We present the X-ray results on the Arches Cluster and G0.1-0.1 cloud obtained with XMM-Newton. In particular we have found a big loop-like annular structure, adjacent to the Arches Cluster, with the diameter of ~3 arcmin (~7 pc) and width of ~1 arcmin (~2 pc). The structure is found to show a non-thermal X-ray spectrum with a best-ftting photon index of Γ = 1.4 ± 0.6, together with a strong fiiorescent Kα line from neutral iron at 6.4-keV with an equivalent width of 1 keV. The G0.1-0.1 cloud shows a reasonable correlation among the 6.4-keV line, very hard continuum and 2.3-keV He-like sulphur line. We discuss the possible origin of these structures and further give a speculation to explain the origin of the fiiorescent X-ray lines in the G...
The Arches cluster is an extraordinarily compact massive star cluster with a core radius of about 10...
The Arches cluster is an extraordinarily compact massive star cluster with a core radius of about 10...
International audienceContext. We present a study of the Arches cluster based on XMM-Newton observat...
Abstract. We present the X-ray results on the Arches Cluster and G0.1−0.1 cloud obtained with XMM-Ne...
The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high l...
The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high l...
International audienceContext. Bright Fe-Kα line emission at 6.4 keV is a unique characteristic of s...
International audienceWe present results of long Nuclear Spectroscopic Telescope Array (NuSTAR; 200 ...
Context. Bright Fe-Kα line emission at 6.4 keV is a unique characteristic of some of the dense molec...
International audienceRecent NuSTAR and XMM–Newton observations of the molecular cloud around the Ar...
Context. The iron Kα line at 6.4 keV provides a valuable spectral diagnostic in several fields of X-...
We present results of long Nuclear Spectroscopic Telescope Array (NuSTAR; 200 ks) and XMM-Newton (10...
The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high l...
The origin of the iron fluorescent line at 6.4 keV from an extended region surrounding the Arches cl...
The Arches cluster is an extraordinarily compact massive star cluster with a core radius of about 10...
The Arches cluster is an extraordinarily compact massive star cluster with a core radius of about 10...
International audienceContext. We present a study of the Arches cluster based on XMM-Newton observat...
Abstract. We present the X-ray results on the Arches Cluster and G0.1−0.1 cloud obtained with XMM-Ne...
The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high l...
The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high l...
International audienceContext. Bright Fe-Kα line emission at 6.4 keV is a unique characteristic of s...
International audienceWe present results of long Nuclear Spectroscopic Telescope Array (NuSTAR; 200 ...
Context. Bright Fe-Kα line emission at 6.4 keV is a unique characteristic of some of the dense molec...
International audienceRecent NuSTAR and XMM–Newton observations of the molecular cloud around the Ar...
Context. The iron Kα line at 6.4 keV provides a valuable spectral diagnostic in several fields of X-...
We present results of long Nuclear Spectroscopic Telescope Array (NuSTAR; 200 ks) and XMM-Newton (10...
The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high l...
The origin of the iron fluorescent line at 6.4 keV from an extended region surrounding the Arches cl...
The Arches cluster is an extraordinarily compact massive star cluster with a core radius of about 10...
The Arches cluster is an extraordinarily compact massive star cluster with a core radius of about 10...
International audienceContext. We present a study of the Arches cluster based on XMM-Newton observat...