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 | The contents of the Gliese 758 B page were merged into Gliese 758 on 3 October 2022. For the contribution history and old versions of the redirected page, please see its history; for the discussion at that location, see its talk page. |
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Merger proposal
editThis binary star system currently has separate articles on the stellar and brown dwarf components. This seems to be because it was initially thought that the brown dwarf might be planetary-mass; certainly articles on exoplanets are very often created separately from (or even instead of) articles on their star systems, but in this case the companion is definitely a brown dwarf. So I propose merging Gliese 758 B into Gliese 758. SevenSpheresCelestia (talk) 18:11, 2 September 2022 (UTC)
- No opposition, will merge. SevenSpheres (talk) 00:25, 4 October 2022 (UTC)