File:Cataclysmic variable.svg
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![File:Cataclysmic variable.svg](https://upload.wikimedia.org/wikipedia/commons/thumb/5/54/Cataclysmic_variable.svg/220px-Cataclysmic_variable.svg.png?20221107103747)
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[edit]DescriptionCataclysmic variable.svg |
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⊙. |
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Source | Own work |
Author | Philip D. Hall |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 10:37, 7 November 2022 | ![]() | 220 × 117 (17 KB) | Bjankuloski06 (talk | contribs) | Wrong place for replacement |
10:35, 7 November 2022 | ![]() | 581 × 243 (27 KB) | Bjankuloski06 (talk | contribs) | Enlargement | |
11:37, 30 November 2016 | ![]() | 220 × 117 (17 KB) | Pdhall99 (talk | contribs) | Tweaks to reduce file size | |
19:41, 13 October 2016 | ![]() | 220 × 117 (33 KB) | Pdhall99 (talk | contribs) | User created page with UploadWizard |
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Width | 220px |
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13 October 2016
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7fdfdaf0863c8070da62feb7d1eb47608a028055
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