Q86934953

Summary

Q86934953 is a long-period variable star^[1].

Key Facts

• Q86934953's instance of is recorded as long-period variable star^[2].
• Q86934953's instance of is recorded as eclipsing binary candidate^[3].
• Q86934953's instance of is recorded as infrared source^[4].
• Q86934953's instance of is recorded as near-infrared source^[5].
• Q86934953's constellation is recorded as Perseus^[6].
• Q86934953's spectral class is recorded as M4^[7].
• Q86934953's catalog code is recorded as 2MASS J04130880+4942350^[8].
• Q86934953's catalog code is recorded as BD+49 1130^[9].
• Q86934953's catalog code is recorded as GSC 03336-00486^[10].
• Q86934953's catalog code is recorded as IRAS 04094+4934^[11].
• Q86934953's catalog code is recorded as NSV 1504^[12].
• Q86934953's catalog code is recorded as Gaia DR2 247322912904363776^[13].
• Q86934953's catalog code is recorded as V481 Per^[14].
• Q86934953's catalog code is recorded as TYC 3336-486-1^[15].
• Q86934953's catalog code is recorded as TIC 267812474^[16].
• Q86934953's catalog code is recorded as DO 28056^[17].
• Q86934953's catalog code is recorded as Gaia DR3 247322912904363776^[18].
• Q86934953's type of variable star is recorded as slow irregular variables of late spectral types^[19].
• Q86934953's type of variable star is recorded as long-period variable star^[20].
• Q86934953's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.78'}^[21].
• Q86934953's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.633'}^[22].
• Q86934953's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.548'}^[23].
• Q86934953's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.038'}^[24].
• Q86934953's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.44'}^[25].
• Q86934953's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.274333'}^[26].

Body

Definition and Type

Recorded instance of include long-period variable star^[2], eclipsing binary candidate^[3], infrared source^[4], and near-infrared source^[5].