| Display title | Astronomy:Delta Scuti variable |
| Default sort key | Delta Scuti variable |
| Page length (in bytes) | 11,683 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374617 |
| Page content language | en - English |
| Page content model | wikitext |
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| Counted as a content page | Yes |
| Page image |  |
| HandWiki item ID | None |
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| Page creator | imported>Sherlock |
| Date of page creation | 08:02, 6 February 2024 |
| Latest editor | imported>Sherlock |
| Date of latest edit | 08:02, 6 February 2024 |
| Total number of edits | 1 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | A Delta Scuti variable (sometimes termed dwarf cepheid when the V-band amplitude is larger than 0.3 mag.) is a subclass of young pulsating star.
These variables as well as classical cepheids are important standard candles and have been used to establish the distance to the Large Magellanic Cloud, globular... |
