Talk:Ursa Major moving group
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Metallicities
[edit]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
[edit] | It is requested that a map or maps be included in this article to improve its quality. Wikipedians in astronomy may be able to help! |
155.192.161.120 (talk) 19:59, 18 November 2010 (UTC)
Stream Data Correction
[edit]HD 26932 should be HD 26923, since the former is in Eridanus and not in Taurus as listed.