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FU Tauri b was nominated for deletion. The discussion was closed on 14 April 2020 with a consensus to merge. Its contents were merged into FU Tauri. The original page is now a redirect to this page. For the contribution history and old versions of the redirected article, please see its history; for its talk page, see here.
The article clearly states that this is a star with a distant gas giant exoplanet, and there is a separate article for the exoplanet. The two peer-reviewed references included in the article both describe it as a brown dwarf binary system. There are web urls for catalogues that include the secondary as a high-mass exoplanet. Which sources are the more reliable? Lithopsian (talk) 14:31, 31 March 2020 (UTC)[reply]
I've listed the exoplanet at AfD, since I don't see it meeting the criteria for notability even if it should be considered to be a planet rather than a brown dwarf. I'm planning to update this article to describe a binary brown dwarf unless anyone objects. Lithopsian (talk) 19:48, 1 April 2020 (UTC)[reply]
Done, and FU Tauri b merged here. Kind of. Since that article was about a gas giant and I couldn't find papers treating it as a gas giant, it is referred to as a brown dwarf in the article. Lithopsian (talk) 18:40, 14 April 2020 (UTC)[reply]
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