EMU discovery of Thunder: a bow-shock PWN powered by PSR J1631-4722 escaping Nimbus SNR (G336.7+0.5)
S. Lazarević, C. Maitra, A. Ahmad, R. Z. E. Alsaberi, S. Dai, D. Leahy, M. D. Filipović, P. G. Edwards, O. Kargaltsev, M. Abdelmaguid, J. D. Gelfand, J. West, S. Hutschenreuter, R. Brose, R. Kothes, V. Velović, C. Burger-Scheidlin, B. D. Ball, G. Graham, A. M. Hopkins, G. P. Rowell, S. F. Rahman, Z. J. Smeaton, S. Taziaux
astro-ph.HE
Submitted: 2026-06-21
Comments: 12 figures, 8 tables. Accepted for publication in ApJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Radio detection of supernova remnant G310.7-5.4 with $\gamma$-ray counterpart: Abeona SNR
- NE2001.I. A New Model for the Galactic Distribution of Free Electrons and its Fluctuations
- Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
- IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament
- Neutron Star Kicks and Supernova Asymmetry
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