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Summary
| Description |
English: The light curve of DQ Herculis, from AAVSO data. The pronounced "dust dip" roughly four months after peak brightness was caused by dust forming as the ejected shell expanded and cooled. |
| Date | |
| Source | Own work |
| Author | PopePompus |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 02:23, 13 December 2020 | | 969 × 630 (67 KB) | PopePompus | Added label to vertical axis |
| 20:32, 6 December 2020 |  | 969 × 630 (61 KB) | PopePompus | Cross-wiki upload from en.wikipedia.org |
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