Classical novae are dramatic stellar explosions with an energy release that is only overcome by supernovae and gamma-ray bursts. These unique cataclysmic events constitute a crucible where different scientific disciplines merge, including astrophysics, nuclear and atomic physics, cosmochemistry, hig
Nova nucleosynthesis
โ Scribed by S. Starrfield; J.W. Truran; M. Wiescher; W.M. Sparks
- Publisher
- Elsevier Science
- Year
- 1997
- Tongue
- English
- Weight
- 238 KB
- Volume
- 621
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
โฆ Synopsis
We report on the results of hydrodynamic calculations, with updated nuclear reaction rates and opacities, which examine the consequences of the accretion process on 1.25M o white dwarfs since that is the most probable mass for the white dwarf in V1974 Cyg 1992.
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Iz quasi-analytic study on ONeMg novae is performed to examine explosive nucleosynthesis in wide range of whit,e dwarf and envelope masses. Comparing our results n-it11 recent) observations enables us to constrain those two parameters. -About a half of Oh served ONeMg novae may have attained high
A quasi-analytic study on ONeMg novae is performed to examine nucleosynthesis in wide range of white dwarf and envelope masses. Comparing our results with recent observations enables us to constrain those two parameters. About a half of observed ONeMg novae may have attained considerably high envelo