Q88858946
carbon star in the constellation Cygnus
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Q88858946
Summary
Q88858946 is a carbon star[1].
Key Facts
- Q88858946's instance of is recorded as carbon star[2].
- Q88858946's instance of is recorded as infrared source[3].
- Q88858946's instance of is recorded as long-period variable star[4].
- Q88858946's instance of is recorded as near-infrared source[5].
- Q88858946's constellation is recorded as Cygnus[6].
- Q88858946's spectral class is recorded as C[7].
- Q88858946's catalog code is recorded as CGCS 4796[8].
- Q88858946's catalog code is recorded as GSC 02684-01641[9].
- Q88858946's catalog code is recorded as IRAS 20152+3643[10].
- Q88858946's catalog code is recorded as 2MASS J20170856+3653130[11].
- Q88858946's catalog code is recorded as MSX6C G074.8061+00.7831[12].
- Q88858946's catalog code is recorded as Gaia DR2 2060562653933154688[13].
- Q88858946's catalog code is recorded as V436 Cyg[14].
- Q88858946's catalog code is recorded as AAVSO 2013+36[15].
- Q88858946's catalog code is recorded as TIC 12024080[16].
- Q88858946's catalog code is recorded as Gaia DR3 2060562653933154688[17].
- Q88858946's type of variable star is recorded as SRa semi-regular variable star[18].
- Q88858946's type of variable star is recorded as long-period variable star[19].
- Q88858946's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.00'}[20].
- Q88858946's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.665'}[21].
- Q88858946's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.292'}[22].
- Q88858946's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.26'}[23].
- Q88858946's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.555874'}[24].
- Q88858946's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.6'}[25].
- Q88858946's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6323'}[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].