Q93904188
classical Cepheid variable star in the constellation Vulpecula
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Q93904188
Summary
Q93904188 is a classical Cepheid variable[1].
Key Facts
- Q93904188's instance of is recorded as classical Cepheid variable[2].
- Q93904188's instance of is recorded as near-infrared source[3].
- Q93904188's instance of is recorded as variable star[4].
- Q93904188's constellation is recorded as Vulpecula[5].
- Q93904188's catalog code is recorded as ASAS J194635+2253.4[6].
- Q93904188's catalog code is recorded as GSC 02139-02370[7].
- Q93904188's catalog code is recorded as HIC 97309[8].
- Q93904188's catalog code is recorded as HIP 97309[9].
- Q93904188's catalog code is recorded as 2MASS J19463518+2253232[10].
- Q93904188's catalog code is recorded as Gaia DR1 1827869808377481216[11].
- Q93904188's catalog code is recorded as Gaia DR2 1827869808377481216[12].
- Q93904188's catalog code is recorded as BR Vul[13].
- Q93904188's catalog code is recorded as AAVSO 1942+22[14].
- Q93904188's catalog code is recorded as TYC 2139-2370-1[15].
- Q93904188's catalog code is recorded as TIC 386383387[16].
- Q93904188's catalog code is recorded as Gaia DR3 1827869808377481216[17].
- Q93904188's type of variable star is recorded as classical Cepheid variable[18].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.019'}[19].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.885'}[20].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.354'}[21].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.136'}[22].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.65'}[23].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.85'}[24].
- Q93904188's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.128908'}[25].
- Q93904188's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4137'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], near-infrared source[3], and variable star[4].