F. Bocchino
Identifiers
- name variant F. Bocchino 0.60 · backfill
Papers (45)
- 3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission astro-ph.HE · 2018 · author #9
- Investigating the Structure of Vela X astro-ph.HE · 2018 · author #7
- Indications of a Si-rich bilateral jet of ejecta in the Vela SNR observed with XMM-Newton astro-ph.HE · 2017 · author #4
- XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction astro-ph.HE · 2016 · author #7
- Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta astro-ph.HE · 2016 · author #4
- Supernova 1987A: a Template to Link Supernovae to their Remnants astro-ph.HE · 2015 · author #4
- The study of neutron star magnetospheres with LOFT astro-ph.HE · 2015 · author #2
- Shock-cloud interaction and particle acceleration in SN 1006 astro-ph.HE · 2014 · author #6
- The loss-limited electron energy in SN 1006: effects of the shock velocity and of the diffusion process astro-ph.HE · 2013 · author #2
- The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton astro-ph.HE · 2013 · author #2
- The Hot and Energetic Universe: The astrophysics of supernova remnants and the interstellar medium astro-ph.HE · 2013 · author #6
- Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant astro-ph.HE · 2013 · author #4
- XMM-Newton and Chandra observations of G272.2-3.2. Evidence of stellar ejecta in the central region astro-ph.HE · 2013 · author #3
- XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration astro-ph.HE · 2012 · author #2
- A population of isolated hard X-ray sources near the supernova remnant Kes 69 astro-ph.HE · 2012 · author #1
- Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of Type Ia supernova remnants astro-ph.HE · 2012 · author #2
- YouASTRO: a web-based bibliography management system with distributed comments and rating features for SAO/NASA ADS papers astro-ph.IM · 2011 · author #1
- Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of supernova remnants astro-ph.HE · 2011 · author #2
- Constraints on local interstellar magnetic field from non-thermal emission of SN1006 astro-ph.HE · 2011 · author #1
- Magnetic fields in supernova remnants and pulsar-wind nebulae astro-ph.GA · 2011 · author #3
- Observational constraints on the modeling of SN1006 astro-ph.HE · 2010 · author #3
- Radio, X-ray and gamma-ray surface brightness profiles as powerful diagnostic tools for non-thermal SNR shells astro-ph.HE · 2010 · author #4
- Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs astro-ph.HE · 2010 · author #3
- Spatial identification of the overionized plasma in W49B astro-ph.HE · 2010 · author #2
- Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants astro-ph.HE · 2010 · author #2
- Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 astro-ph.HE · 2009 · author #2
- Some properties of synchrotron radio and inverse-Compton gamma-ray images of supernova remnants astro-ph.HE · 2009 · author #3
- On the metal abundances inside mixed-morphology supernova remnants: the case of IC443 and G166.0+4.3 astro-ph.GA · 2009 · author #1
- Aspect angle for interstellar magnetic field in SN 1006 astro-ph · 2008 · author #4
- The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds astro-ph · 2008 · author #2
- Physical and chemical inhomogeneities inside the Vela SNR shell. Indications of ejecta shrapnels astro-ph · 2007 · author #2
- Science with the new generation high energy gamma- ray experiments astro-ph · 2007 · author #21
- On the Origin of Asymmetries in Bilateral Supernova Remnants astro-ph · 2007 · author #2
- A physical interpretation of the jet-like X-ray emission from supernova remnant W49B astro-ph · 2007 · author #4
- Shock-cloud interaction in the Vela SNR II. Hydrodynamic model astro-ph · 2006 · author #4
- Crushing of interstellar gas clouds in supernova remnants II. X-ray emission astro-ph · 2006 · author #2
- XMM-Newton observations of the supernova remnant IC443: I. soft X-ray emission from shocked interstellar medium astro-ph · 2006 · author #2
- The X-ray emission of the supernova remnant W49B observed with XMM-Newton astro-ph · 2006 · author #4
- Shock-cloud interaction in the Vela SNR observed with XMM-Newton astro-ph · 2005 · author #2
- Crushing of interstellar gas clouds in supernova remnants. I. The role of thermal conduction and radiative losses astro-ph · 2005 · author #4
- Hard Extended X-ray Source in the IC 443 SNR Resolved by Chandra: A Fast Ejecta Fragment or a New Pulsar Wind Nebula? astro-ph · 2005 · author #2
- The extended hard X-ray emission from the Vela Plerion astro-ph · 2005 · author #3
- The X-ray Halo of G21.5-0.9 astro-ph · 2003 · author #2
- BeppoSAX observation of the composite remnant G327.1-1.1 astro-ph · 2002 · author #1
- Modeling Non-Confined Coronal Flares: Dynamics and X-Ray Diagnostics astro-ph · 2001 · author #2
Mentions
- 1401.7196 #6 · backfill · confidence 0.70 F. Bocchino
- 1309.1414 #2 · backfill · confidence 0.70 F. Bocchino
- 1306.6048 #2 · backfill · confidence 0.70 F. Bocchino
- 1306.2335 #6 · backfill · confidence 0.70 F. Bocchino
- 1301.3085 #4 · backfill · confidence 0.70 F. Bocchino
- 1301.1507 #3 · backfill · confidence 0.70 F. Bocchino
- 1208.5966 #2 · backfill · confidence 0.70 F. Bocchino
- 1204.3470 #1 · backfill · confidence 0.70 F. Bocchino
- 1202.3593 #2 · backfill · confidence 0.70 F. Bocchino
- 1112.0329 #1 · backfill · confidence 0.70 F. Bocchino
- 1109.0192 #2 · backfill · confidence 0.70 F. Bocchino
- 1105.2689 #1 · backfill · confidence 0.70 F. Bocchino
- 1104.4047 #3 · backfill · confidence 0.70 F. Bocchino
- 1012.4586 #3 · backfill · confidence 0.70 F. Bocchino
- 1012.4579 #4 · backfill · confidence 0.70 F. Bocchino
- 1011.1847 #3 · backfill · confidence 0.70 F. Bocchino
- 1004.1604 #2 · backfill · confidence 0.70 F. Bocchino
- 1001.2240 #2 · backfill · confidence 0.70 F. Bocchino
- 0903.3392 #2 · backfill · confidence 0.70 F. Bocchino
- 0901.4258 #3 · backfill · confidence 0.70 F. Bocchino
- 0901.3228 #1 · backfill · confidence 0.70 F. Bocchino
- 0811.2319 #4 · backfill · confidence 0.70 F. Bocchino
- 0801.1403 #2 · backfill · confidence 0.70 F. Bocchino
- 0712.3017 #2 · backfill · confidence 0.70 F. Bocchino
- 0712.1548 #21 · backfill · confidence 0.70 F. Bocchino
- 0704.0890 #2 · backfill · confidence 0.70 F. Bocchino
Frequent Coauthors
- M. Miceli 28 shared papers
- S. Orlando 25 shared papers
- F. Reale 13 shared papers
- O. Petruk 11 shared papers
- A. Decourchelle 8 shared papers
- G. Peres 8 shared papers
- J. Ballet 4 shared papers
- J. Vink 4 shared papers
- M.L. Pumo 4 shared papers
- G. Cusumano 3 shared papers
- G. Dubner 3 shared papers
- R. Petre 3 shared papers
- S. Broersen 3 shared papers
- T. Mineo 3 shared papers
- V. Beshley 3 shared papers
- A. Bamba 2 shared papers
- A. Pellizzoni 2 shared papers
- A. Tiengo 2 shared papers
- D. Iakubovskyi 2 shared papers
- E. Massaro 2 shared papers