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138 results on '"Bucciantini N"'

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1. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

3. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

4. Uncovering the geometry of the hot X-ray corona in the seyfert galaxy NGC 4151 with IXPE

5. X-ray polarimetry and spectroscopy of the neutron star low-mass X-ray binary GX 9+9: an in-depth study with IXPE and NuSTAR

6. Complex variations of X-ray polarization in the X-ray pulsar LS V +44 17/RX J0440.9+4431

7. X-ray polarimetry of X-ray pulsar X Persei: another orthogonal rotator?

8. Uncovering the geometry of the hot X-ray corona in the Seyfert galaxy NGC4151 with IXPE

9. Reverberation of pulsar wind nebulae – III. Modelling of the plasma interface empowering a long term radiative evolution.

10. Multi-messenger and transient astrophysics with the Cherenkov Telescope Array

11. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

12. Reverberation of pulsar wind nebulae – II. Anatomy of the 'thin-shell' evolution.

13. The LOFT Mission Concept - A Status Update

16. Characterization of the Optical and X-ray Properties of the Northwestern Wisps in the Crab Nebula

17. Spatially-resolved Spectroscopy of the IC443 Pulsar Wind Nebula and Environs

18. Modelling the γ-ray pulsar wind nebulae population in our galaxy.

19. Revisiting the evolution of non-radiative supernova remnants: a hydrodynamical-informed parametrization of the shock positions.

20. Future X-ray Polarimetry of Relativistic Accelerators: PWNe and SNRs

21. XIPE: the x-ray imaging polarimetry explorer

22. Reverberation of pulsar wind nebulae (I): impact of the medium properties and other parameters upon the extent of the compression.

23. Axisymmetric equilibrium models for magnetised neutron stars in scalar-tensor theories.

24. XIPE

25. Deciphering the nature of the pulsar wind nebula CTB 87 with XMM–Newton.

26. General relativistic magnetohydrodynamic dynamo in thick accretion discs: fully non-linear simulations.

27. On the origin of jet-like features in bow shock pulsar wind nebulae.

28. Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: emission and polarization.

29. Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: dynamics.

30. XIPE: the X-ray imaging polarimetry explorer

31. Probing the emission physics and weak/soft population of Gamma-Ray Bursts with LOFT

32. Dynamo action in thick disks around Kerr black holes: high-order resistive GRMHD simulations

33. High-order schemes for non-ideal $3+1$ GRMHD: a study of the kinematic dynamo process in accretion tori

34. The Large Observatory for x-ray timingSpace Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray

35. Review of the Theory of PWNe

36. Numerical simulations of mass loading in the tails of bow-shock pulsar-wind nebulae.

37. Escape of high-energy particles from bow-shock pulsar wind nebulae.

38. Modeling radio circular polarization in the Crab nebula.

39. Papaloizou-Pringle instability suppression by the magnetorotational instability in relativistic accretion discs.

40. CTA contributions to the 33rd International Cosmic Ray Conference

41. Short GRBs with Extended Emission from Magnetar Birth: Jet Formation and Collimation

42. The Proto-Magnetar Model for Gamma-Ray Bursts

43. GRMHD in axisymmetric dynamical spacetimes: the X-ECHO code

44. MHD models of Pulsar Wind Nebulae

45. Unveiling the Magnetic Structure of VHE SNRs/PWNe with XIPE, the X-ray Imaging-Polarimetry Explorer.

46. MHD Models for Winds from Neutron Stars, and their Interaction with the Environment

47. Polarization properties of turbulent synchrotron bubbles: an approach based on Chandrasekhar-Kendall functions.

48. Modeling the effect of small-scale magnetic turbulence on the X-ray properties of Pulsar Wind Nebulae.

49. General relativistic models for rotating magnetized neutron stars in conformally flat space-time.

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