- Review on particle acceleration in SNRs
- Reynolds 2008, Blasi 2013, Cristofari et al. 2021, Vink 2021 (springer, book)
- Engel et al. 2022: multimessenger science in the next decade
- Becker Tjus 2020: Review of cosmic rays
- SN1987A X-ray analyses
- e.g., Park et al. 2011, Sun et al. 2021, Greco et al. 2022
- Long et al. 2022: simulations of rotating stars, dredging up of C, N, O
- Ho et al. 2021: cooling of CCOs
- Wu et al. 2021: how to create CCOs
- CCO list by De Luca at http://www.iasf-milano.inaf.it/~deluca/cco/main.htm
- Olausen et al. 2014: magnetar catalog
- SNR-HMXB lists, how to create such systems: Khokhriakova et al. 2022
- Proper motion measurements for several CCOs: Mayer et al. 2021
- XINSs vs. magnetars: Yoneyama et al. 2019
- XINSs are old magnetars ?
- Comparison of magnetar hosting SNRs and those with ordinary PSRs
- Martin et al. 2014
- no difference
- SNR-NS systems, initial spins: Popov et al. 2012
- covers only ~half of SNR-NS systems know in 2022
- Birth kick of neutron stars: Ng et al. 2007
- PeVatrons simulations within 14 days after a SN: Inoue et al. 2021
- Fugaku simulations
- Kinematic study of CCOs and SNRs
- rapid expansion of G350.1-0.3
- RX J1713’s kinematic age
- LHAASO detection of 12 objects in TeV–PeV
- almost no SNRs
- one is completely unidentified
- Magnetar model, age estimation
- age estimation –> really ?
- Radiation from failed SNe
- 1e-4 to 1e-3 of typical SNe’s ejected energies
- small size < 10 pc, slow shocks < 1000 km s-1
- seen in soft X-rays
- < a few sources in LMC by eROSITA
- SRG and early results
- eROSITA all sky picture
- Neutrino mass is less than 1 eV ?
- KATRIN experiment
- electron-capture SN is possible and NS is formed
- paper
- Prof. Nomoto at Kavli IPMU
- Crab nebula is explained
- Hitomi background origins
- Galactic diffuse TeV with Fermi
- Review of pulsars
- by Teruaki Enoto
- NS kicks and SN ejecta distribution
- X-ray IME by imaging spectroscopy
- explosion center = geometric center
- anti-correlation between IME vs. NS directions
- HESS search for gamma-rays from runway stars
- upper limits = 0.1– 1 % of kinetic energies
- Geminga gamma-rays with HAWC
- Diffuse Galactic gamma-rays with HESS
- NS kicks and SN asymmetry
- asymmetry by shell shapes
- anti-correlation between IME vs. NS directions
- SNR physics in X-rays
- by Jacco Vink
- Shock heating with presence of acceleration
- by Jacco Vink et al.
- Shock velocity vs. T_p/T_e ratio
- T_p/T_e \propto v^-2 ?
- (simple) theory: T_p/T_e = m_p/m_e (const.)
H. Suzuki's Astrophysical Studies 