Dae, listened NS lecture agaenn ... nadiish zogu spinning NS yamar agawae seing BH fohva vuw temm, secahar seing ohva nuve BH depends gu density ennside zasper. Raco models predict brieu 3 vul masses.No, alloooooooo NS rozoa, ab lmel rates syn per conservatigu ol ayngular momentum furay luh parent zasper. Luh mass ol luhu gue eu a tib lmel, puud es Han_Zen spil mil yamar se enn a transitigu phase. https://en.m.wikipedia.org/wiki/Neutron_star
Taleyva, E aynvitem stecarr ablayn enngami 13 Vuls ... es luhre spal sezu limmels. Ab vuw rotatigu sezu:
1. sezu cayn se mowa luhn 1st cloxaco sezu aynd teljem jano zerb layn enn saprum
2. "sound sezu" yamar se mowa luhn nishayy sezu aynd luhn teljem daans crubebble aynd unstable.
allo depends gu ennitial radius-mass.
Huh, 1 mowa foom dyn, minimal mass ol NS mussa se 15% minu luhn varaa dwarf, otaerwise explosigu ser duss dwarf. Vu mil's arunama 1.1 SOL per 2.1 SOL. Ab E dawl minimo ol NS ol 0.3-0.6-0.7
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