RXJ2129-z8HeII
The purpose of this redirect is currently being discussed by the Wikipedia community. The outcome of the discussion may result in a change of this page, or possibly its deletion in accordance with Wikipedia's deletion policy. Please share your thoughts on the matter at this redirect's entry on the Redirects for discussion page. Click on the link below to go to the current destination page. Please notify the good-faith creator and any main contributors of the redirect by placing {{subst:Rfd notice|RXJ2129-z8HeII}} ~~~~ on their talk page. |
This title is currently a redirect to Stellar population#Population III stars; click there to go to the current target. The full content of this redirect page, including all redirect categories, is displayed below. |
#REDIRECT Stellar population#Population III stars
NOTE: The "RXJ2129-z8HeII" Redirect to "Population III stars" was based on an astronomical study published in the responsible scientific literature[1] - hope this helps in some way - in any case - Stay Safe and Healthy !! - Drbogdan (talk) 00:12, 12 May 2024 (UTC)
References
- ^ Wang, Xin; et al. (8 December 2022). "A strong He II λ1640 emitter with extremely blue UV spectral slope at z=8.16: presence of Pop III stars?". arxiv. Archived from the original on 11 May 2024. Retrieved 11 May 2024.