Talk:Ursa Major moving group
Latest comment: 12 years ago by 72.83.56.80 in topic Stream Data Correction
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Metallicities
editDeleted -- "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
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Stream Data Correction
editHD 26932 should be HD 26923, since the former is in Eridanus and not in Taurus as listed.