| Display title | Astronomy:Helium star |
| Default sort key | Helium star |
| Page length (in bytes) | 4,278 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375392 |
| 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 |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>MainAI6 |
| Date of page creation | 12:02, 6 February 2024 |
| Latest editor | imported>MainAI6 |
| Date of latest edit | 12:02, 6 February 2024 |
| 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. | A helium star is a class O or B star (blue), which has extraordinarily strong helium lines and weaker than normal hydrogen lines, indicating strong stellar winds and a mass loss of the outer envelope. Extreme helium stars (EHe) entirely lack hydrogen in their spectra. Pure helium stars lie on or near... |
