Thermal Processes in Supernova Remnants
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Publisher
Springer Nature Singapore
Link
https://link.springer.com/content/pdf/10.1007/978-981-19-6960-7_89
Reference24 articles.
1. Y. Amano, H. Uchida, T. Tanaka, L. Gu, T.G. Tsuru, Evidence for resonance scattering in the x-ray grating spectrum of the supernova remnant N49. Astrophys. J. 897, 12 (2020). https://doi.org/10.3847/1538-4357/ab90fc
2. M. Balikhin, M. Gedalin, A. Petrukovich, New mechanism for electron heating in shocks. Phys. Rev. Lett. 70, 1259 (1993). https://doi.org/10.1103/PhysRevLett.70.1259
3. P.J. Cargill, K. Papadopoulos, A mechanism for strong shock electron heating in supernova remnants. Astrophys. J. 329, L29 (1988). https://doi.org/10.1086/185170
4. P. Ghavamian, J.M. Laming, C.E. Rakowski, A physical relationship between electron-proton temperature equilibration and mach number in fast collisionless shocks. Astrophys. J. 654, L69 (2007). https://doi.org/10.1086/510740
5. P. Ghavamian, S.J. Schwartz, J. Mitchell, A. Masters, J.M. Laming, Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection Space Science Reviews 178, 633 (2013). https://doi.org/10.1007/s11214-013-9999-0
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