Revision as of 10:45, 23 March 2015 edit Praemonitus (talk \| contribs) Autopatrolled, Extended confirmed users 65,682 edits →61 Cygni ← Previous edit		Revision as of 10:46, 23 March 2015 edit undo Praemonitus (talk \| contribs) Autopatrolled, Extended confirmed users 65,682 edits →61 Cygni Next edit →
Line 45: :::::: Yes, the absence of a detectable IR excess is still of interest because it tells the reader something about the state of the system. The reference for the habitability radii is in a separate bullet above. [[User:Praemonitus\|Praemonitus]] ([[User talk:Praemonitus\|talk]]) :::::::I think the same is explained in ''Refining planetary boundaries'' section. Right? -[[User:The Herald\|The Herald]] [[User talk:The Herald\|<sup style="margin-left:0.5px">''the joy of the LORD''</sup>]][[Special:Contributions/The Herald\|<sub style="margin-left:-47.5px">''my strength''</sub>]] 07:51, 23 March 2015 (UTC) :::::::: Nope. That only covers the topic of detection of planets, not an IR excess due to an circumstellar disk. [[User:Praemonitus\|Praemonitus]] ([[User talk:Praemonitus\|talk]]) 10:45, 23 March 2015 (UTC) Thanks. [[User:Praemonitus\|Praemonitus]] ([[User talk:Praemonitus\|talk]]) 16:20, 18 March 2015 (UTC)

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