HD54399

Summary

HD54399 is a peculiar star^[1].

Key Facts

• HD54399's instance of is recorded as peculiar star^[2].
• HD54399's instance of is recorded as Alpha² Canum Venaticorum variable^[3].
• HD54399's instance of is recorded as infrared source^[4].
• HD54399's constellation is recorded as Carina^[5].
• HD54399's spectral class is recorded as ApSr(CrEu)^[6].
• HD54399's catalog code is recorded as HD 54399^[7].
• HD54399's catalog code is recorded as CPC 20.1 1715^[8].
• HD54399's catalog code is recorded as GSC 08908-00183^[9].
• HD54399's catalog code is recorded as 2MASS J07043873-6150381^[10].
• HD54399's catalog code is recorded as PPM 355807^[11].
• HD54399's catalog code is recorded as SAO 249725^[12].
• HD54399's catalog code is recorded as TIC 348898673^[13].
• HD54399's catalog code is recorded as TYC 8908-183-1^[14].
• HD54399's catalog code is recorded as Gaia DR1 5287007022280635264^[15].
• HD54399's catalog code is recorded as Gaia DR2 5287007022280635264^[16].
• HD54399's type of variable star is recorded as Alpha² Canum Venaticorum variable^[17].
• HD54399's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.97'}^[18].
• HD54399's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.72'}^[19].
• HD54399's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7552'}^[20].
• HD54399's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.302'}^[21].
• HD54399's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.208'}^[22].
• HD54399's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.149'}^[23].
• HD54399's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4006'}^[24].
• HD54399's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+713.9797'}^[25].
• HD54399's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+106.16139746741780'}^[26].

Body

Definition and Type

Recorded instance of include peculiar star^[2], Alpha² Canum Venaticorum variable^[3], and infrared source^[4].