Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well understood. Several remnants present distorted radio or X-ray shells with jet-like structures. G290.1-0.8 (MSH 11-61A) belongs to this particular class. Aims. We aim to investigate the nature of this supernova remnant in order to unveil the origin of its particular morphology. We based our work on the study of the X-ray emitting plasma properties and the conditions imposed by the cold interstellar medium where the remnant expanded. Methods. We use archival radio, H I line data and X-ray observations from XMM-Newton and Chandra observatories, to study G290.1-0.8 and its surrounding medium in detail. Spatially resolved spectral analysis and mea...
Aims. We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5-5.6 throu...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well un...
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well un...
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well un...
We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with comple...
We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with comple...
G290.1-0.8 (MSH 11-61A) is a supernova remnant (SNR) whose X-ray morphology is centrally bright. How...
Aims. We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high en...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Due to its centrally bright X-ray morphology and limb brightened radio profile, MSH 11–61A (G290.1–0...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5-5.6 throu...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well un...
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well un...
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well un...
We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with comple...
We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with comple...
G290.1-0.8 (MSH 11-61A) is a supernova remnant (SNR) whose X-ray morphology is centrally bright. How...
Aims. We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high en...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Due to its centrally bright X-ray morphology and limb brightened radio profile, MSH 11–61A (G290.1–0...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5-5.6 throu...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray ...