File:Chi Cygni near minima in visible light and infrared.jpg
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Summary
| Description |
English: Chi Cygni near its minimum brightness in visible light and 1µm infrared light. The spectacular reduction in visible magnitude is largely caused by a shift in the peak emission wavelength towards the infrared during its cycle. As a result, when viewed in infrared light, the star is quite bright even at minima. |
| Date | |
| Source | Own work |
| Author | Timwether |
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| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 01:22, 8 August 2022 | 1,416 × 1,014 (286 KB) | Timwetherell | Uploaded own work with UploadWizard |
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