Q89776003

Summary

Q89776003 is a long-period variable star^[1].

Key Facts

• Q89776003's instance of is recorded as long-period variable star^[2].
• Q89776003's instance of is recorded as infrared source^[3].
• Q89776003's instance of is recorded as near-infrared source^[4].
• Q89776003's constellation is recorded as Taurus^[5].
• Q89776003's spectral class is recorded as M5^[6].
• Q89776003's catalog code is recorded as 2MASS J05410509+1635299^[7].
• Q89776003's catalog code is recorded as BD+16 840^[8].
• Q89776003's catalog code is recorded as GSC 01298-00853^[9].
• Q89776003's catalog code is recorded as IRAS 05381+1634^[10].
• Q89776003's catalog code is recorded as Gaia DR2 3396569023693469568^[11].
• Q89776003's catalog code is recorded as DX Tau^[12].
• Q89776003's catalog code is recorded as TYC 1298-853-1^[13].
• Q89776003's catalog code is recorded as UBV M 751^[14].
• Q89776003's catalog code is recorded as TIC 59215150^[15].
• Q89776003's catalog code is recorded as Gaia DR3 3396569023693469568^[16].
• Q89776003's type of variable star is recorded as slow irregular variables of late spectral types^[17].
• Q89776003's type of variable star is recorded as long-period variable star^[18].
• Q89776003's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.33'}^[19].
• Q89776003's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.30'}^[20].
• Q89776003's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.828'}^[21].
• Q89776003's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.835'}^[22].
• Q89776003's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.520'}^[23].
• Q89776003's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.212311'}^[24].
• Q89776003's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6899'}^[25].
• Q89776003's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+37.52'}^[26].

Body

Definition and Type

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