File:Formation of disks around white dwarfs.jpg
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Summary[edit]
DescriptionFormation of disks around white dwarfs.jpg |
English: I created this graph by using the sublimation radius and Roche Limit of G29-38 as mentioned in Steckloff et al. 2021. This graph was inspired and is based partially on Figure 5 of Veras et al. 2024, but contains realistic sizes of the white dwarf, Roche Limit and Sublimation radius. The size of the minor planet is exaggerated. The circular shape of the debris at the "Tidal Disruption"-stage is based on simulations by Veras et al. 2017 |
Date | |
Source | Own work |
Author | Meli thev |
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I, the copyright holder of this work, hereby publish it under the following license:
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Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 16:01, 29 February 2024 | 2,359 × 2,611 (575 KB) | Meli thev (talk | contribs) | Uploaded own work with UploadWizard |
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Orientation | Normal |
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Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Software used | Adobe Photoshop Elements 12.0 Windows |
File change date and time | 16:37, 29 February 2024 |
Color space | sRGB |
Date metadata was last modified | 17:37, 29 February 2024 |
Date and time of digitizing | 17:04, 29 February 2024 |
Unique ID of original document | xmp.did:E2D1AD81FAD6EE119312EDD86C942111 |
IIM version | 110 |
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