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Aydi, E · 2018 · DOI 10.1093/mnras/stx2678

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astro-ph.SR 1

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2025 1

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CONDITIONAL 1

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The orbital period changes for novae

astro-ph.SR · 2025-07-30 · conditional · novelty 6.0

Binary-driven mass loss during nova eruptions can explain nearly all observed orbital period changes of normal cataclysmic variables, while fast winds alone cannot.

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  • The orbital period changes for novae astro-ph.SR · 2025-07-30 · conditional · none · ref 5

    Binary-driven mass loss during nova eruptions can explain nearly all observed orbital period changes of normal cataclysmic variables, while fast winds alone cannot.