Supernova remnants, planetary nebulae and superbubbles: prospects for new XMM-Newton observations
arXiv:0802.0360 · doi:10.1002/asna.200710907
Abstract
Important results achieved over the last years on supernova remnants, planetary nebulae and superbubbles are briefly reviewed in the context of X-ray observations. I intend to review the important open scientific questions in these fields, and the specific contributions that can be made by XMM-Newton.
4 pages, 1 figure, invited review for "XMM-Newton: The next decade", AN in press
References in corpus (28)
- The Interstellar Environment of our Galaxy
- On the magnetic fields and particle acceleration in Cas A
- Nucleosynthesis and Mixing in Cassiopeia A
- Cosmic Ray Acceleration at the Forward Shock in Tycho's Supernova Remnant: Evidence from Chandra X-ray Observations
- A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with H.E.S.S
- A Million-Second Chandra View of Cassiopeia A
- A Spatial and Spectral Study of Nonthermal Filaments in Historical Supernova Remnants: Observational Results with Chandra
- A Physical Relationship Between Electron-Proton Temperature Equilibration and Mach Number in Fast Collisionless Shocks
- Superbubbles and Energetic Particles in the Galaxy. I: Collective effects of particle acceleration
- Rayleigh-Taylor Instabilities in Young Supernova Remnants Undergoing Efficient Particle Acceleration
- A Deep Chandra Observation of Kepler's Supernova Remnant: A Type Ia Event with Circumstellar Interaction
- XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
- Thermal X-ray Emission and Cosmic Ray Production in Young Supernova Remnants
- Electron Heating and Cosmic Rays at a Supernova Shock from Chandra X-ray Observations of E0102.2-7219
- The blast wave of Tycho's supernova remnant
- Slow Temperature Equilibration Behind the Shock Front of SN 1006
- XMM-Newton observation of the Tycho Supernova Remnant
- XMM-Newton observation of Kepler's supernova remnant
- Hydrodynamic Simulation of Supernova Remnants Including Efficient Particle Acceleration
- From the Owl to the Eskimo: the Radiation-Gasdynamics of Planetary Nebulae IV
- Thermal and Non-thermal X-Rays from the LMC Super Bubble 30 Dor C
- Energy Crisis in the Superbubble DEM L 192 (N 51D)
- The first broad-band X-ray images and spectra of the 30 Doradus region in the LMC
- Confronting the Superbubble Model with X-ray Observations of 30 Dor C
- X-ray emission from Planetary Nebulae. I. Spherically symmetric numerical simulations
- Spatially Resolved X-ray Spectroscopy of Vela Shrapnel A
- Suzaku Reveals Helium-burning Products in the X-ray Emitting Planetary Nebula BD+303639
- X-Ray Emission from Planetary Nebulae Calculated by 1D Spherical Numerical Simulations