Q79951672
carbon star in the constellation Centaurus
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Q79951672
Summary
Q79951672 is a carbon star[1].
Key Facts
- Q79951672's instance of is recorded as carbon star[2].
- Q79951672's instance of is recorded as infrared source[3].
- Q79951672's instance of is recorded as long-period variable star[4].
- Q79951672's instance of is recorded as near-infrared source[5].
- Q79951672's constellation is recorded as Centaurus[6].
- Q79951672's spectral class is recorded as C[7].
- Q79951672's catalog code is recorded as CGCS 3485[8].
- Q79951672's catalog code is recorded as IRAS 14156-5645[9].
- Q79951672's catalog code is recorded as NSV 6614[10].
- Q79951672's catalog code is recorded as ASAS J141910-5659.6[11].
- Q79951672's catalog code is recorded as [W71b] 094-04[12].
- Q79951672's catalog code is recorded as 2MASS J14190982-5659406[13].
- Q79951672's catalog code is recorded as Gaia DR2 5892277904145922176[14].
- Q79951672's catalog code is recorded as V1341 Cen[15].
- Q79951672's catalog code is recorded as Gaia DR3 5892277904145922176[16].
- Q79951672's catalog code is recorded as TIC 413285371[17].
- Q79951672's type of variable star is recorded as long-period variable star[18].
- Q79951672's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.50'}[19].
- Q79951672's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.72'}[20].
- Q79951672's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.071'}[21].
- Q79951672's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.591'}[22].
- Q79951672's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.947'}[23].
- Q79951672's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.765859'}[24].
- Q79951672's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.58'}[25].
- Q79951672's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1724.138'}[26].
Body
Definition and Type
Recorded instance of include carbon star[2], infrared source[3], long-period variable star[4], and near-infrared source[5].