Q86119835
rotating variable star in the constellation Canes Venatici
Press Enter · cited answer in seconds
0 sources
Q86119835
Summary
Q86119835 is a rotating variable star[1].
Key Facts
- Q86119835's instance of is recorded as rotating variable star[2].
- Q86119835's constellation is recorded as Canes Venatici[3].
- Q86119835's spectral class is recorded as G0[4].
- Q86119835's catalog code is recorded as [ZEH2003] RX J1346.0+4201 1[5].
- Q86119835's catalog code is recorded as AG+42 1236[6].
- Q86119835's catalog code is recorded as BD+42 2437[7].
- Q86119835's catalog code is recorded as GSC 03029-00340[8].
- Q86119835's catalog code is recorded as PPM 53727[9].
- Q86119835's catalog code is recorded as RBS 1312[10].
- Q86119835's catalog code is recorded as RX J1346.0+4201[11].
- Q86119835's catalog code is recorded as SAO 44739[12].
- Q86119835's catalog code is recorded as TYC 3029-340-1[13].
- Q86119835's catalog code is recorded as 2MASS J13460148+4201080[14].
- Q86119835's catalog code is recorded as 1RXS J134601.2+420108[15].
- Q86119835's catalog code is recorded as ASAS J134601+4201.1[16].
- Q86119835's catalog code is recorded as Gaia DR1 1500689748208519296[17].
- Q86119835's catalog code is recorded as Gaia DR2 1500689752504456576[18].
- Q86119835's type of variable star is recorded as rotating variable star[19].
- Q86119835's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.492'}[20].
- Q86119835's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.972'}[21].
- Q86119835's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.841'}[22].
- Q86119835's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.18'}[23].
- Q86119835's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.24'}[24].
- Q86119835's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9799'}[25].
- Q86119835's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.3684'}[26].
Body
Definition and Type
Q86119835's instance of is recorded as rotating variable star[2].