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Summary
| Description |
English: Schematic of a non-magnetic cataclysmic variable. A white dwarf (on the right) accretes matter through an accretion disk, fed by a Roche-lobe-filling main-sequence donor star (on the left). Matter from the donor star travels in a stream from the Lagrange point L1 and meets the accretion disk at a hot spot.
The white dwarf has a mass of 0.8 M⊙, its companion is a main sequence star of 0.5 M⊙ and their centres are separated by 1.64 R⊙. |
| Date | |
| Source | Own work |
| Author | Philip D. Hall |
| Other versions |
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File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 10:37, 7 November 2022 | | 220 × 117 (17 KB) | Bjankuloski06 | Wrong place for replacement |
| 10:35, 7 November 2022 |  | 581 × 243 (27 KB) | Bjankuloski06 | Enlargement | |
| 11:37, 30 November 2016 |  | 220 × 117 (17 KB) | Pdhall99 | Tweaks to reduce file size | |
| 19:41, 13 October 2016 |  | 220 × 117 (33 KB) | Pdhall99 | User created page with UploadWizard |
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