File:Binary star system - semidetached configuration q=3 reverse.svg
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[edit]DescriptionBinary star system - semidetached configuration q=3 reverse.svg |
English: Schematic of a binary star system in a semidetached configuration with a mass ratio q=3, viewed at an inclination of 90 degrees (edge on). The filled regions represent the two stars. The black line represents the inner critical Roche equipotential, made up of two Roche lobes that meet at the Lagrangian point L1. In a semidetached configuration one star fills its Roche lobe. |
Date | |
Source | Own work |
Author | Philip D. Hall |
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[edit]I, the copyright holder of this work, hereby publish it under the following license:
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 11:47, 16 October 2016 | 198 × 138 (11 KB) | Pdhall99 (talk | contribs) | User created page with UploadWizard |
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Width | 158pt |
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Height | 110pt |
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16 October 2016
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889624ba564f9b77091bd8556cdc6872705893c8
10,753 byte
138 pixel
198 pixel
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