Q79098191

Summary

Q79098191 is a RV Tauri variable^[1].

Key Facts

• Q79098191's instance of is recorded as RV Tauri variable^[2].
• Q79098191's instance of is recorded as infrared source^[3].
• Q79098191's instance of is recorded as long-period variable star^[4].
• Q79098191's instance of is recorded as near-infrared source^[5].
• Q79098191's instance of is recorded as classical Cepheid variable^[6].
• Q79098191's constellation is recorded as Crux^[7].
• Q79098191's spectral class is recorded as M^[8].
• Q79098191's catalog code is recorded as IRAS 12043-5904^[9].
• Q79098191's catalog code is recorded as 2MASS J12065601-5921271^[10].
• Q79098191's catalog code is recorded as Gaia DR2 6070968261816221696^[11].
• Q79098191's catalog code is recorded as AU Cru^[12].
• Q79098191's catalog code is recorded as TIC 67133604^[13].
• Q79098191's catalog code is recorded as UCAC4 154-090349^[14].
• Q79098191's catalog code is recorded as Gaia DR3 6070968261816221696^[15].
• Q79098191's type of variable star is recorded as classical Cepheid variable^[16].
• Q79098191's type of variable star is recorded as RV Tauri variable^[17].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.722'}^[18].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.961'}^[19].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.143'}^[20].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.957947'}^[21].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.106'}^[22].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.71'}^[23].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.445'}^[24].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.155'}^[25].
• Q79098191's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.996'}^[26].

Body

Definition and Type

Recorded instance of include RV Tauri variable^[2], infrared source^[3], long-period variable star^[4], near-infrared source^[5], and classical Cepheid variable^[6].