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	This article was accepted on 31 May 2012 by reviewer Graeme Bartlett (talk · contribs).

Revised age from 2017 publication

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Latest comment: 6 years ago1 comment1 person in discussion

From http://iopscience.iop.org/article/10.3847/1538-4357/aa62a5/meta:

Simultaneously fitting for both disk components, we derive ages of 6.8–7.0 Gyr for the thin disk and 8.7 ± 0.1 Gyr for the thick disk from the local 40 pc sample. Similarly, we derive ages of 7.4–8.2 Gyr for the thin disk and 9.5–9.9 Gyr for the thick disk from the deep proper motion catalog, which shows no evidence of a deviation from a constant star formation rate in the past 2.5 Gyr.

24.69.131.109 (talk) 07:20, 30 September 2018 (UTC)Reply

Wiki Education Foundation-supported course assignment

Latest comment: 2 years ago1 comment1 person in discussion

This article is or was the subject of a Wiki Education Foundation-supported course assignment. Further details are available on the course page. Student editor(s): Master of Chaldea. Peer reviewers: Ccoakley.

Above undated message substituted from Template:Dashboard.wikiedu.org assignment by PrimeBOT (talk) 12:28, 18 January 2022 (UTC)Reply

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Talk:Thin disk

Revised age from 2017 publication

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Wiki Education Foundation-supported course assignment