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| Main Authors: | , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2501.07067 |
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| _version_ | 1866929673825419264 |
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| author | Vathachira, Irin Babu Hillman, Yael Kashi, Amit |
| author_facet | Vathachira, Irin Babu Hillman, Yael Kashi, Amit |
| contents | We define two regimes of the parameter space of symbiotic systems based on the dominant mass transfer mechanism. A wide range of white dwarf (WD) mass, donor mass, and donor radius combinations are explored to determine the separation, for each parameter combination, below which wind Roche-lobe overflow (WRLOF) will be the dominant mass transfer mechanism. The underlying concept is the premise that the wind accelerates. If it reaches the Roche-lobe before attaining sufficient velocity to escape, it will be trapped, and gravitationally focused through the inner Lagrangian point towards the accreting WD. However, if the wind succeeds in attaining the required velocity to escape from the donor's Roche-lobe, it will disperse isotropically, and the dominant mass transfer mechanism will be the Bondi-Hoyle-Lyttleton (BHL) prescription in which only a fraction of the wind will be accreted onto the WD. We present, these two regimes of the four dimensional parameter space, covering 375 different parameter combinations. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_07067 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Exploring mass transfer mechanisms in symbiotic systems Vathachira, Irin Babu Hillman, Yael Kashi, Amit Solar and Stellar Astrophysics High Energy Astrophysical Phenomena We define two regimes of the parameter space of symbiotic systems based on the dominant mass transfer mechanism. A wide range of white dwarf (WD) mass, donor mass, and donor radius combinations are explored to determine the separation, for each parameter combination, below which wind Roche-lobe overflow (WRLOF) will be the dominant mass transfer mechanism. The underlying concept is the premise that the wind accelerates. If it reaches the Roche-lobe before attaining sufficient velocity to escape, it will be trapped, and gravitationally focused through the inner Lagrangian point towards the accreting WD. However, if the wind succeeds in attaining the required velocity to escape from the donor's Roche-lobe, it will disperse isotropically, and the dominant mass transfer mechanism will be the Bondi-Hoyle-Lyttleton (BHL) prescription in which only a fraction of the wind will be accreted onto the WD. We present, these two regimes of the four dimensional parameter space, covering 375 different parameter combinations. |
| title | Exploring mass transfer mechanisms in symbiotic systems |
| topic | Solar and Stellar Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2501.07067 |