@article{oai:ir.soken.ac.jp:00004260,
 author = {池内, 了 and IKEUCHI, Satoru and NAKAZAWA, Kiyoshi and MURAI, Tadayuki and HOSHI, Reiun and HAYASHI, Chushiro},
 issue = {6},
 journal = {Progress of Theoretical Physics, Progress of Theoretical Physics},
 month = {},
 note = {As a continuation of the preceding paper, the evolution of carbon-oxygen stars of 1.5M⊙ and 2.6M⊙ has been computed from a pre-carbon-burning stage to a pre-supernova stage for the two alternative cases, with and without neutrino loss. 

In the case without neutrinos, it has been found that after the termination of central carbon-burning electrons become degenerate at the center and both neon-burning and siliconburning begin as strong flashes. Finally, both of the stars become dynamically unstable on account of the photo-disintegration of iron. 

In the case with neutrinos, the inversion of temperature gradient occurs in stages after central carbon-burning. This is due to the effect of neutrino loss coupled with the effect of electron degeneracy. Finally, the 1.5M⊙ star and the 2.6M⊙ star become unstable on account of the inverse-beta process of silicon and the photo-disintegration of iron, respectively.},
 pages = {1870--1884},
 title = {Stellar Evolution toward Pre-Supernova Stage. II},
 volume = {48},
 year = {1972}
}