Q85572860

Summary

Q85572860 is a rotating variable star^[1].

Key Facts

• Q85572860's instance of is recorded as rotating variable star^[2].
• Q85572860's instance of is recorded as BY Draconis variable^[3].
• Q85572860's instance of is recorded as near-infrared source^[4].
• Q85572860's instance of is recorded as astrophysical X-ray source^[5].
• Q85572860's constellation is recorded as Vulpecula^[6].
• Q85572860's catalog code is recorded as 2MASS J20390464+2338471^[7].
• Q85572860's catalog code is recorded as 1RXS J203905.4+233845^[8].
• Q85572860's catalog code is recorded as ASAS J203905+2338.7^[9].
• Q85572860's catalog code is recorded as Gaia DR2 1819161092169985664^[10].
• Q85572860's catalog code is recorded as UCAC4 569-110547^[11].
• Q85572860's catalog code is recorded as V504 Vul^[12].
• Q85572860's catalog code is recorded as Gaia DR3 1819161092169985664^[13].
• Q85572860's catalog code is recorded as TIC 243539190^[14].
• Q85572860's catalog code is recorded as TYC 2170-326-1^[15].
• Q85572860's type of variable star is recorded as rotating variable star^[16].
• Q85572860's type of variable star is recorded as BY Draconis variable^[17].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.38'}^[18].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.142'}^[19].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.660'}^[20].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.548'}^[21].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.778'}^[22].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.689'}^[23].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.54'}^[24].
• Q85572860's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.557914'}^[25].
• Q85572860's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.2317'}^[26].

Body

Definition and Type

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