File:RW Cephei extended mid-infrared emission.png
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Summary
| Description |
English: RW Cephei is a hypergiant which has undergone an enhanced mass loss phase ending less than 100 years ago. The material released by the star causes it to appear extended in mid-infrared wavelengths. This image shows the extent of the circumstellar material seen at a wavelength of 11.9 μm. |
| Date | |
| Source | https://iopscience.iop.org/article/10.3847/2515-5172/acd37f |
| Author | Terry Jay Jones |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 17:05, 16 May 2023 | | 858 × 858 (245 KB) | Nussun05 | Uploaded a work by Terry Jay Jones from https://iopscience.iop.org/article/10.3847/2515-5172/acd37f with UploadWizard |
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