V894 Herculis

Summary

V894 Herculis is a long-period variable star^[1].

Key Facts

• V894 Herculis's instance of is recorded as long-period variable star^[2].
• V894 Herculis's instance of is recorded as spectroscopic binary^[3].
• V894 Herculis's constellation is recorded as Hercules^[4].
• V894 Herculis's spectral class is recorded as K0^[5].
• V894 Herculis's catalog code is recorded as ASAS J162335+2103.3^[6].
• V894 Herculis's catalog code is recorded as GSC 01517-01071^[7].
• V894 Herculis's catalog code is recorded as HD 147866^[8].
• V894 Herculis's catalog code is recorded as HIC 80302^[9].
• V894 Herculis's catalog code is recorded as HIP 80302^[10].
• V894 Herculis's catalog code is recorded as IRAS 16214+2110^[11].
• V894 Herculis's catalog code is recorded as PPM 104841^[12].
• V894 Herculis's catalog code is recorded as 1RXS J162335.4+210320^[13].
• V894 Herculis's catalog code is recorded as SAO 84343^[14].
• V894 Herculis's catalog code is recorded as UCAC4 556-056975^[15].
• V894 Herculis's catalog code is recorded as YZ 21 5591^[16].
• V894 Herculis's catalog code is recorded as AG+21 1599^[17].
• V894 Herculis's catalog code is recorded as BD+21 2913^[18].
• V894 Herculis's catalog code is recorded as [ZEH2003] RX J1623.5+2103 1^[19].
• V894 Herculis's catalog code is recorded as RX J1623.5+2103^[20].
• V894 Herculis's catalog code is recorded as Gaia DR1 1298185270016868736^[21].
• V894 Herculis's catalog code is recorded as Gaia DR2 1298185274313671424^[22].
• V894 Herculis's catalog code is recorded as V894 Her^[23].
• V894 Herculis's catalog code is recorded as Gaia DR3 1298185274313671424^[24].
• V894 Herculis's catalog code is recorded as TYC 1517-1071-1^[25].
• V894 Herculis's type of variable star is recorded as rotating variable star^[26].

Body

Designation and Status

Recorded instance of include long-period variable star^[2] and spectroscopic binary^[3].

History and Context

Catalog codes include ASAS J162335+2103.3^[6], GSC 01517-01071^[7], HD 147866^[8], HIC 80302^[9], HIP 80302^[10], and IRAS 16214+2110^[11].