转换 发表于 2025-3-26 22:49:37

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轻率的你 发表于 2025-3-27 02:30:52

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Armory 发表于 2025-3-27 09:19:43

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优雅 发表于 2025-3-27 10:16:52

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坚毅 发表于 2025-3-27 16:02:24

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prostatitis 发表于 2025-3-27 20:38:31

CNO Abundances and Nova Outburst Strengths,, deduced from the accretion disk luminosity, is too high to permit a strong enough hydrogen flash to give the observed nova strength. Some possible resolutions to this paradox are suggested..Recurrent novae are probably not themonuclear runaways on accreting white dwarfs.

callous 发表于 2025-3-28 01:43:48

The Formation of Optical CNO Emission Lines in Cataclysmic Variables,nes of carbon are also present in old novae, probably formed by recombination processes. The available data for the optical CNO lines suggest that non-solar CNO enhancements exist in quiescent novae, indicating that some of the binary systems may be evolved.

让空气进入 发表于 2025-3-28 02:11:13

Optimal Control Under Stochastic Uncertainty, deduced from the accretion disk luminosity, is too high to permit a strong enough hydrogen flash to give the observed nova strength. Some possible resolutions to this paradox are suggested..Recurrent novae are probably not themonuclear runaways on accreting white dwarfs.

Tracheotomy 发表于 2025-3-28 10:03:39

Controlled Random Search Under Uncertaintynes of carbon are also present in old novae, probably formed by recombination processes. The available data for the optical CNO lines suggest that non-solar CNO enhancements exist in quiescent novae, indicating that some of the binary systems may be evolved.

ARIA 发表于 2025-3-28 11:11:27

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查看完整版本: Titlebook: Cataclysmic Variables and Related Objects; Proceedings of the 7 Mario Livio,Giora Shaviv Conference proceedings 1983 D. Reidel Publishing C