Q86464285

Summary

Q86464285 is an emission-line star^[1].

Key Facts

• Q86464285's instance of is recorded as emission-line star^[2].
• Q86464285's instance of is recorded as long-period variable star^[3].
• Q86464285's instance of is recorded as infrared source^[4].
• Q86464285's instance of is recorded as near-infrared source^[5].
• Q86464285's constellation is recorded as Camelopardalis^[6].
• Q86464285's spectral class is recorded as M6III^[7].
• Q86464285's catalog code is recorded as 2MASS J03402518+6046517^[8].
• Q86464285's catalog code is recorded as GSC 04062-01834^[9].
• Q86464285's catalog code is recorded as IRAS 03362+6037^[10].
• Q86464285's catalog code is recorded as Gaia DR2 474411092401097728^[11].
• Q86464285's catalog code is recorded as FZ Cam^[12].
• Q86464285's catalog code is recorded as TIC 392372990^[13].
• Q86464285's catalog code is recorded as Gaia DR3 474411092401097728^[14].
• Q86464285's type of variable star is recorded as long-period variable star^[15].
• Q86464285's type of variable star is recorded as semiregular variable star^[16].
• Q86464285's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.309'}^[17].
• Q86464285's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.048'}^[18].
• Q86464285's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.593'}^[19].
• Q86464285's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.443013'}^[20].
• Q86464285's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6415'}^[21].
• Q86464285's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1558.846'}^[22].
• Q86464285's SIMBAD ID is recorded as V* FZ Cam^[23].
• Q86464285's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.10507751823'}^[24].
• Q86464285's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+60.78103337431'}^[25].
• Q86464285's epoch is recorded as J2000.0^[26].