Q82531292
long period variable
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Q82531292
Summary
Q82531292 is a long-period variable star[1].
Key Facts
- Q82531292's instance of is recorded as long-period variable star[2].
- Q82531292's instance of is recorded as infrared source[3].
- Q82531292's instance of is recorded as near-infrared source[4].
- Q82531292's constellation is recorded as Sagitta[5].
- Q82531292's spectral class is recorded as K[6].
- Q82531292's catalog code is recorded as BD+17 4061[7].
- Q82531292's catalog code is recorded as HD 350430[8].
- Q82531292's catalog code is recorded as IRAS 19407+1806[9].
- Q82531292's catalog code is recorded as 2MASS J19425669+1813524[10].
- Q82531292's catalog code is recorded as Gaia DR2 1824183871803031424[11].
- Q82531292's catalog code is recorded as CV Sge[12].
- Q82531292's catalog code is recorded as AAVSO 1938+18[13].
- Q82531292's catalog code is recorded as UBV M 859[14].
- Q82531292's catalog code is recorded as TYC 1606-172-1[15].
- Q82531292's catalog code is recorded as TIC 359798490[16].
- Q82531292's catalog code is recorded as Gaia DR3 1824183871803031424[17].
- Q82531292's type of variable star is recorded as slow irregular variables of late spectral types[18].
- Q82531292's type of variable star is recorded as long-period variable star[19].
- Q82531292's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.69'}[20].
- Q82531292's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.710'}[21].
- Q82531292's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.731'}[22].
- Q82531292's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.03'}[23].
- Q82531292's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.291'}[24].
- Q82531292's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.289206'}[25].
- Q82531292's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7972'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].