65 citations
- Consejo Nacional de Investigaciones Científicas y TécnicasAR17 papers
- Universidad Complutense de MadridES12 papers
- Universidad Nacional de La PlataAR12 papers
- Bariloche Atomic CentreAR8 papers
- Instituto Argentino de RadioastronomíaAR8 papers
- Osservatorio Astronomico di PalermoIT8 papers
- Universidad de JaénES7 papers
- Balseiro InstituteAR5 papers
- Comisión Nacional de Energía AtómicaAR3 papers
- National Institute for AstrophysicsIT3 papers
- University of PalermoIT3 papers
- Institute of Astronomy and Space PhysicsAR2 papers
7 papers · 1 filter
XMM-Newton and Chandra observations of G272.2-3.2. Evidence of stellar ejecta in the central region
E. Sánchez-Ayaso, J. A. Combi, F. Bocchino +4
We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant G272.2-3.2, in order to get important constra…
On the origin of the jet-like radio/X-ray morphology of G290.1-0.8
Federico García, Jorge A. Combi, Juan F. Albacete-Colombo +3
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 structur…
AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
J. Lopez-Santiago, M. Miceli, M. V. del Valle +6
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway star…
A multiwavelength study of the supernova remnant G296.8-0.3
E. Sánchez-Ayaso, J. A. Combi, J. F. Albacete Colombo +3
We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with complementary radio and infrared data. The spatial and spectral properties of the X-ra…
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)
J. A. Combi, J. F. Albacete Colombo, E. Sanchez-Ayaso +6
Aims. We report the first detailed X-ray study of the supernova remnant (SNR) G304.6+0.1, achieved with the XMM-Newton mission. Methods. The powerful imaging capability of XMM-Newt…
An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302
J. A. Combi, J. F. Albacete Colombo, J. Lopez-Santiago +7
Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-like X-ray source located at the geometrical center of the SNR radio structure. Me…