V939 Herculis

Summary

V939 Herculis is a long-period variable star^[1].

Key Facts

• V939 Herculis's instance of is recorded as long-period variable star^[2].
• V939 Herculis's instance of is recorded as infrared source^[3].
• V939 Herculis's instance of is recorded as near-infrared source^[4].
• V939 Herculis's constellation is recorded as Hercules^[5].
• V939 Herculis's spectral class is recorded as Mb^[6].
• V939 Herculis's catalog code is recorded as DO 15828^[7].
• V939 Herculis's catalog code is recorded as GSC 03077-00997^[8].
• V939 Herculis's catalog code is recorded as HD 155523^[9].
• V939 Herculis's catalog code is recorded as HIC 84004^[10].
• V939 Herculis's catalog code is recorded as HIP 84004^[11].
• V939 Herculis's catalog code is recorded as IRAS 17086+4045^[12].
• V939 Herculis's catalog code is recorded as IRC +40292^[13].
• V939 Herculis's catalog code is recorded as 2MASS J17101852+4041238^[14].
• V939 Herculis's catalog code is recorded as PPM 55971^[15].
• V939 Herculis's catalog code is recorded as RAFGL 1929^[16].
• V939 Herculis's catalog code is recorded as SAO 46531^[17].
• V939 Herculis's catalog code is recorded as AG+40 1574^[18].
• V939 Herculis's catalog code is recorded as BD+40 3110^[19].
• V939 Herculis's catalog code is recorded as Gaia DR2 1353910619553212928^[20].
• V939 Herculis's catalog code is recorded as V939 Her^[21].
• V939 Herculis's catalog code is recorded as TIC 85407251^[22].
• V939 Herculis's catalog code is recorded as Gaia DR3 1353910619553212928^[23].
• V939 Herculis's catalog code is recorded as AAVSO 1707+40^[24].
• V939 Herculis's catalog code is recorded as TYC 3077-997-1^[25].
• V939 Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.25'}^[26].

Body

Designation and Status

Recorded instance of include long-period variable star^[2], infrared source^[3], and near-infrared source^[4].

History and Context

Catalog codes include DO 15828^[7], GSC 03077-00997^[8], HD 155523^[9], HIC 84004^[10], HIP 84004^[11], and IRAS 17086+4045^[12].