File:PHL 5038AB system.jpg
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Size of this preview: 800 × 452 pixels. Other resolutions: 320 × 181 pixels | 640 × 362 pixels | 1,024 × 579 pixels | 1,280 × 723 pixels | 3,508 × 1,982 pixels.
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Summary[edit]
| Description |
English: I created this diagram displaying the hypothetical evolution of the PHL 5038AB system according to Casewell et al. 2024: https://arxiv.org/abs/2404.05488
I use here the case of a circular orbit for the brown dwarf to simplify the diagram. The outer stable edge of the disk around the white dwarf is here assumed to be 24.5 AU (in between the 17-32 AU outer edge mentioned in the paper). The outer stable edge would be 5-6 AU for an elliptical orbit of the brown dwarf. |
| 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:
This file is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.
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- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 14:29, 10 April 2024 | | 3,508 × 1,982 (497 KB) | Meli thev (talk | contribs) | some improvements: gradual size increase of the orbits and "debris belt" instead of "debris disk" |
| 11:28, 10 April 2024 |  | 3,508 × 1,982 (497 KB) | Meli thev (talk | contribs) | correction: not separation, but semi-major axis | |
| 19:38, 9 April 2024 |  | 3,508 × 1,982 (494 KB) | Meli thev (talk | contribs) | Uploaded own work with UploadWizard |
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