Q84497187
long period variable
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Q84497187
Summary
Q84497187 is a long-period variable star[1].
Key Facts
- Q84497187's instance of is recorded as long-period variable star[2].
- Q84497187's instance of is recorded as infrared source[3].
- Q84497187's instance of is recorded as near-infrared source[4].
- Q84497187's constellation is recorded as Centaurus[5].
- Q84497187's catalog code is recorded as GSC 08650-00956[6].
- Q84497187's catalog code is recorded as IRAS 12301-5422[7].
- Q84497187's catalog code is recorded as NSV 5700[8].
- Q84497187's catalog code is recorded as 2MASS J12325446-5438539[9].
- Q84497187's catalog code is recorded as UCAC2 8035109[10].
- Q84497187's catalog code is recorded as Gaia DR1 6074526796836030848[11].
- Q84497187's catalog code is recorded as Gaia DR2 6074526801150659968[12].
- Q84497187's catalog code is recorded as V1126 Cen[13].
- Q84497187's catalog code is recorded as TYC 8650-956-1[14].
- Q84497187's catalog code is recorded as UBV M 6634[15].
- Q84497187's catalog code is recorded as TIC 272908080[16].
- Q84497187's catalog code is recorded as Gaia DR3 6074526801150659968[17].
- Q84497187's type of variable star is recorded as slow irregular variables of late spectral types[18].
- Q84497187's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.18'}[19].
- Q84497187's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.1'}[20].
- Q84497187's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.151'}[21].
- Q84497187's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.298'}[22].
- Q84497187's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.956'}[23].
- Q84497187's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.039677'}[24].
- Q84497187's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5727'}[25].
- Q84497187's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.08'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].