File:HR4049LightCurve.png
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Summary
| Description |
English: A light curve for HR 4049. The main plot shows the V band variation over one orbital period. The inset plot shows that the amplitude of the light curve decreases at longer observing wavelengths, because the opacity of the dust decreases. Adapted from Jorissen & Frankowski (2008) DOI: 10.1063/1.2999998 |
| Date | |
| Source | Own work |
| Author | PopePompus |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 04:12, 14 October 2021 | | 1,500 × 975 (118 KB) | PopePompus | Cross-wiki upload from en.wikipedia.org |
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