- PeVatrons simulations within 14 days after a SN
- Inoue et al.
- 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
— 2020 —
- 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
— 2019 — - Review of pulsars
- by Teruaki Enoto
— 2018 —
- 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
— older —
- 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.)
-
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H. Suzuki's Astrophysical Studies 