Q95942398

Summary

Q95942398 is a hot subdwarf star^[1].

Key Facts

• Q95942398's instance of is recorded as hot subdwarf star^[2].
• Q95942398's instance of is recorded as near-infrared source^[3].
• Q95942398's constellation is recorded as Aquarius^[4].
• Q95942398's spectral class is recorded as sdB^[5].
• Q95942398's child astronomical body is recorded as PHL 457 b^[6].
• Q95942398's catalog code is recorded as uvby98 610061110^[7].
• Q95942398's catalog code is recorded as 2MASS J23192442-0852379^[8].
• Q95942398's catalog code is recorded as UCAC2 28839481^[9].
• Q95942398's catalog code is recorded as UCAC4 406-141392^[10].
• Q95942398's catalog code is recorded as Gaia DR2 2438094814718695424^[11].
• Q95942398's catalog code is recorded as DENIS J231924.4-085237^[12].
• Q95942398's catalog code is recorded as Gaia DR3 2438094814718695424^[13].
• Q95942398's catalog code is recorded as TIC 49590066^[14].
• Q95942398's type of variable star is recorded as rotating variable star^[15].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.78'}^[16].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.95'}^[17].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.499'}^[18].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.595'}^[19].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.674'}^[20].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.27'}^[21].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.179'}^[22].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.168'}^[23].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.764'}^[24].
• Q95942398's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.919305'}^[25].
• Q95942398's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.39'}^[26].

Body

Definition and Type

Recorded instance of include hot subdwarf star^[2] and near-infrared source^[3].