Edge Rewrite
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a229b4217b41b86e

Jump to content

Talk:Kepler-421

Page contents not supported in other languages.
Add topic
From Wikipedia, the free encyclopedia
Latest comment: 3 years ago by Lithopsian in topic KOI-1274 B association with KOI-1274 A

KOI-1274 B association with KOI-1274 A

[edit]

Currently the article claims that the secondary star KOI-1274 B is not associated with KOI-1274 A, but the distance of the secondary star in the paper that this statement is referring to, considering its large error range, is consistent with that of the primary, and the low (0.87) certainty of physical unassociatedness in the paper suggests that the companion is likely physically associated with the primary. AstroChara (talk) 01:10, 19 May 2023 (UTC)Reply

So about 60% likelihood of being unassociated? Being consistent, within the margins of error, simply means it could be associated, not that it is. Lithopsian (talk) 13:22, 19 May 2023 (UTC)Reply