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Talk:Ursa Major moving group

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Metallicities

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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)[reply]

Chart would be good

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155.192.161.120 (talk) 19:59, 18 November 2010 (UTC)[reply]

Stream Data Correction

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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)[reply]