Citation: I. Hachisu et M. Kato, Recurrent novae as a progenitor system of Type Ia supernovae. I. RS Ophiuchi subclass: Systems with a red giant companion, ASTROPHYS J, 558(1), 2001, pp. 323-350
Citation: I. Hachisu et M. Kato, Prediction of the supersoft X-ray phase, helium enrichment, and turnoff time in the 2000 outburst of the recurrent nova CI Aquilae, ASTROPHYS J, 553(2), 2001, pp. L161-L164
Citation: I. Hachisu et al., A new evolutionary path to type Ia supernovae: A helium-rich supersoft X-ray source channel, ASTROPHYS J, 519(1), 1999, pp. 314-323
Citation: I. Hachisu et M. Kato, A new interpretation for the second peak of T Coronae Borealis outbursts: A tilting disk around a very massive white dwarf, ASTROPHYS J, 517(1), 1999, pp. L47-L50
Citation: M. Kato et I. Hachisu, A new estimation of mass accumulation efficiency in helium shell flashes toward Type Ia supernova explosions, ASTROPHYS J, 513(1), 1999, pp. L41-L44
Authors:
Kobayashi, C
Tsujimoto, T
Nomoto, K
Hachisu, I
Kato, M
Citation: C. Kobayashi et al., Low-metallicity inhibition of type Ia supernovae and galactic and cosmic chemical evolution, ASTROPHYS J, 503(2), 1998, pp. L155-L159