Q79626219

Summary

Q79626219 is a rotating variable star^[1].

Key Facts

• Q79626219's instance of is recorded as rotating variable star^[2].
• Q79626219's instance of is recorded as BY Draconis variable^[3].
• Q79626219's instance of is recorded as near-infrared source^[4].
• Q79626219's instance of is recorded as astrophysical X-ray source^[5].
• Q79626219's instance of is recorded as young stellar object candidate^[6].
• Q79626219's constellation is recorded as Crux^[7].
• Q79626219's spectral class is recorded as K5IVe^[8].
• Q79626219 is part of Scorpius–Centaurus Association^[9].
• Q79626219's catalog code is recorded as 1RXS J115948.2-613618^[10].
• Q79626219's catalog code is recorded as GSC 08973-01607^[11].
• Q79626219's catalog code is recorded as ASAS J115948-6136.2^[12].
• Q79626219's catalog code is recorded as UCAC4 142-091776^[13].
• Q79626219's catalog code is recorded as 2MASS J11594986-6136246^[14].
• Q79626219's catalog code is recorded as Gaia DR2 5335087948554484352^[15].
• Q79626219's catalog code is recorded as FM Cru^[16].
• Q79626219's catalog code is recorded as Gaia DR3 5335087948554484352^[17].
• Q79626219's catalog code is recorded as TIC 307889317^[18].
• Q79626219's type of variable star is recorded as rotating variable star^[19].
• Q79626219's type of variable star is recorded as BY Draconis variable^[20].
• Q79626219's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.407'}^[21].
• Q79626219's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.13'}^[22].
• Q79626219's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.59'}^[23].
• Q79626219's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.55'}^[24].
• Q79626219's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.88'}^[25].
• Q79626219's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.51'}^[26].

Body

Definition and Type

Recorded instance of include rotating variable star^[2], BY Draconis variable^[3], near-infrared source^[4], astrophysical X-ray source^[5], and young stellar object candidate^[6].

Use and Application

Q79626219 is part of Scorpius–Centaurus Association^[9].