| Display title | Astronomy:BL Herculis variable |
| Default sort key | BL Herculis variable |
| Page length (in bytes) | 4,822 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 373954 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>WikiGary |
| Date of page creation | 00:17, 24 October 2022 |
| Latest editor | imported>WikiGary |
| Date of latest edit | 00:17, 24 October 2022 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | BL Herculis variables are a subclass of type II Cepheids with low luminosity and mass, that have a period of less than eight days. They are pulsating stars with light curves that frequently show a bump on the descending side for stars of the shortest periods and on the ascending side for longer period... |
