HT Кассиопеи

Summary

HT Кассиопеи is a binary star^[1].

Key Facts

• HT Кассиопеи's instance of is recorded as binary star^[2].
• HT Кассиопеи's instance of is recorded as spectroscopic binary^[3].
• HT Кассиопеи's instance of is recorded as cataclysmic variable star^[4].
• HT Кассиопеи's instance of is recorded as astrophysical X-ray source^[5].
• HT Кассиопеи's instance of is recorded as emission-line star^[6].
• HT Кассиопеи's instance of is recorded as near-infrared source^[7].
• HT Кассиопеи's constellation is recorded as Cassiopeia^[8].
• HT Кассиопеи's spectral class is recorded as M5.5e^[9].
• HT Кассиопеи's catalog code is recorded as 2MASS J01101312+6004354^[10].
• HT Кассиопеи's catalog code is recorded as HT Cas^[11].
• HT Кассиопеи's catalog code is recorded as 1RXS J011013.6+600431^[12].
• HT Кассиопеи's catalog code is recorded as SBC9 59^[13].
• HT Кассиопеи's catalog code is recorded as WEB 1208^[14].
• HT Кассиопеи's catalog code is recorded as Gaia DR2 426306363477869696^[15].
• HT Кассиопеи's catalog code is recorded as AAVSO 0103+59^[16].
• HT Кассиопеи's catalog code is recorded as TIC 52861041^[17].
• HT Кассиопеи's catalog code is recorded as Gaia DR3 426306363477869696^[18].
• HT Кассиопеи's type of variable star is recorded as SU Ursae Majoris variable^[19].
• HT Кассиопеи's type of variable star is recorded as eclipsing binary star^[20].
• HT Кассиопеи's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.703'}^[21].
• HT Кассиопеи's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.226'}^[22].
• HT Кассиопеи's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.843'}^[23].
• HT Кассиопеи's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.313334'}^[24].
• HT Кассиопеи's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1'}^[25].
• HT Кассиопеи's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.936508'}^[26].

Body

Definition and Type

Recorded instance of include binary star^[2], spectroscopic binary^[3], cataclysmic variable star^[4], astrophysical X-ray source^[5], emission-line star^[6], and near-infrared source^[7].