Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Share This Author
The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
- K. Nandra, D. Barret, I. Zhuravleva
- Physics
- 1 June 2013
This White Paper, submitted to the recent ESA call for science themes to define its future large missions, advocates the need for a transformational leap in our understanding of two key questions in…
XMM-Newton observations of the supernova remnant IC 443: II. evidence of stellar ejecta in the inner regions.
- E. Troja, F. Bocchino, M. Miceli, F. Reale
- Physics
- 7 April 2008
Aims. We investigate the spatial distribution of the physical and chemical properties of the hot X-ray emitting plasma of the supernova remnant IC 443, in order to get important constraints on its…
Spatial identification of the overionized plasma in W49B
- M. Miceli, F. Bocchino, A. Decourchelle, J. Ballet, F. Reale
- Physics
- 9 April 2010
Context. Recent Suzaku X-ray observations of the ejecta-dominated supernova remnant W49B have shown that there is a clear indication in the global spectrum for overionized plasma, whose physical…
The X-ray emission of the supernova remnant W49B observed with XMM-Newton
- M. Miceli, A. Decourchelle, R. Petre
- Physics
- 23 February 2006
Context. In the framework of the study of supernova remnants and their complex interaction with the interstellar medium, we report on an XMM-Newton EPIC observation of the Galactic supernova remnant…
On the metal abundances inside mixed-morphology supernova remnants: the case of IC 443 and G166.0+4.3
- F. Bocchino, M. Miceli, E. Troja
- Physics
- 21 January 2009
Context. Recent developments in the study of mixed morphology supernova remnants (MMSNRs) have revealed the presence of metal-rich X-ray emitting plasma inside a fraction of these remnants, a feature…
Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
- S. Orlando, M. Miceli, M. L. Pumo, F. Bocchino
- Physics, Geology
- 11 March 2016
The remnants of core-collapse supernovae (SNe) have complex morphologies that may reflect asymmetries and structures developed during the progenitor SN explosion. Here we investigate how the…
Role of Ejecta Clumping and Back-reaction of Accelerated Cosmic Rays in the Evolution of Type Ia Supernova Remnants
- S. Orlando, F. Bocchino, M. Miceli, O. Petruk, M. L. Pumo
- Physics
- 16 February 2012
We investigate the role played by initial clumping of ejecta and by efficient acceleration of cosmic rays (CRs) in determining the density structure of the post-shock region of a Type Ia supernova…
Detailed study of SNR G306.3-0.9 using XMM-Newton and Chandra observations
- J. Combi, F. Garc'ia, A. E. Su'arez, P. Luque-Escamilla, S. Paron, M. Miceli
- Physics
- 29 June 2016
We used combined data from XMM-Newton and Chandra observatories to study the X-ray morphology of SNR G306.3-0.9. A spatially-resolved spectral analysis was used to obtain physical and geometrical…
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single-star and Binary Merger Progenitor Models for SN 1987A
- M. Ono, S. Nagataki, M. Miceli
- PhysicsThe Astrophysical Journal
- 4 December 2019
We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernova) models and…
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006
- M. Miceli, F. Bocchino, G. Castelletti
- Physics
- 19 March 2009
Context. Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006. Aims. We…
...
1
2
3
4
5
...