CO Ursae Majoris

Summary

CO Ursae Majoris is a long-period variable star^[1].

Key Facts

• CO Ursae Majoris's instance of is recorded as long-period variable star^[2].
• CO Ursae Majoris's instance of is recorded as infrared source^[3].
• CO Ursae Majoris's instance of is recorded as near-infrared source^[4].
• CO Ursae Majoris's constellation is recorded as Ursa Major^[5].
• CO Ursae Majoris's spectral class is recorded as C-rich^[6].
• CO Ursae Majoris's catalog code is recorded as FK5 2892^[7].
• CO Ursae Majoris's catalog code is recorded as GCRV 6858^[8].
• CO Ursae Majoris's catalog code is recorded as GSC 02522-02244^[9].
• CO Ursae Majoris's catalog code is recorded as HD 96813^[10].
• CO Ursae Majoris's catalog code is recorded as HIC 54522^[11].
• CO Ursae Majoris's catalog code is recorded as HIP 54522^[12].
• CO Ursae Majoris's catalog code is recorded as HR 4333^[13].
• CO Ursae Majoris's catalog code is recorded as IRAS 11065+3634^[14].
• CO Ursae Majoris's catalog code is recorded as IRC +40222^[15].
• CO Ursae Majoris's catalog code is recorded as 2MASS J11091910+3618336^[16].
• CO Ursae Majoris's catalog code is recorded as PPM 75704^[17].
• CO Ursae Majoris's catalog code is recorded as RAFGL 1462^[18].
• CO Ursae Majoris's catalog code is recorded as SAO 62427^[19].
• CO Ursae Majoris's catalog code is recorded as AG+36 1051^[20].
• CO Ursae Majoris's catalog code is recorded as BD+37 2162^[21].
• CO Ursae Majoris's catalog code is recorded as WEB 9840^[22].
• CO Ursae Majoris's catalog code is recorded as Gaia DR2 762126970124609408^[23].
• CO Ursae Majoris's catalog code is recorded as CO UMa^[24].
• CO Ursae Majoris's catalog code is recorded as AAVSO 1103+36^[25].
• CO Ursae Majoris's catalog code is recorded as GC 15334^[26].

Body

Designation and Status

Recorded instance of include long-period variable star^[2], infrared source^[3], and near-infrared source^[4].

History and Context

Catalog codes include FK5 2892^[7], GCRV 6858^[8], GSC 02522-02244^[9], HD 96813^[10], HIC 54522^[11], and HIP 54522^[12].