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Sub-brown dwarf: Revision history


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18 August 2024

17 August 2024

  • curprev 00:0200:02, 17 August 2024Stevinger talk contribs 11,151 bytes −88 For WD 0806-661 B, DT Virginis c, HD 106906 b, ROXs 42Bb even a 13 MJ companion would have a mass ratio < 0.04 to the primary. The companions are either planets if < 13 MJ or brown dwarfs if > 13 MJ. For FW Tauri b the best solution for the companion found is a 0.1 Msol star. None of the objects previously given is a sub-brown dwarf. Removing all 5. undo Tag: Visual edit: Switched

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