Talk:Ursa Major moving group

Metallicities
Deleted -- "It is believed that the stars in the Ursa Major moving group share a certain chemical signature that may have been characteristic of the nebula from which they were formed: higher than expected levels of barium but lower than expected levels of copper, with a normal abundance of iron for Population I stars." : I couldn't verify this in the technical literature David s graff 03:36, 18 March 2006 (UTC)

Chart would be good
155.192.161.120 (talk) 19:59, 18 November 2010 (UTC)

Stream Data Correction
HD 26932 should be HD 26923, since the former is in Eridanus and not in Taurus as listed.

72.83.56.80 (talk) 06:31, 7 October 2012 (UTC)