Q86844006

Summary

Q86844006 is a rotating variable star^[1].

Key Facts

• Q86844006's instance of is recorded as rotating variable star^[2].
• Q86844006's instance of is recorded as star^[3].
• Q86844006's instance of is recorded as near-infrared source^[4].
• Q86844006's instance of is recorded as double star^[5].
• Q86844006's constellation is recorded as Lyra^[6].
• Q86844006's spectral class is recorded as G1^[7].
• Q86844006's child astronomical body is recorded as Q28855966^[8].
• Q86844006 comprises ** KOI 1061A^[9].
• Q86844006 comprises ** KOI 1061B^[10].
• Q86844006's catalog code is recorded as WDS J19205+4123AB^[11].
• Q86844006's catalog code is recorded as KOI-1061^[12].
• Q86844006's catalog code is recorded as KIC 6037187^[13].
• Q86844006's catalog code is recorded as 2MASS J19203156+4122534^[14].
• Q86844006's catalog code is recorded as UCAC4 657-071343^[15].
• Q86844006's catalog code is recorded as TIC 122298563^[16].
• Q86844006's catalog code is recorded as Kepler-759^[17].
• Q86844006's type of variable star is recorded as rotating variable star^[18].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.327'}^[19].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.009'}^[20].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.967'}^[21].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.29'}^[22].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.40'}^[23].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.87'}^[24].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.65'}^[25].
• Q86844006's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.28'}^[26].

Body

Definition and Type

Recorded instance of include rotating variable star^[2], star^[3], near-infrared source^[4], and double star^[5].

Use and Application

Components include ** KOI 1061A^[9], a star^[27] and ** KOI 1061B^[10], a star^[28].