Q88914789
long period variable
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Q88914789
Summary
Q88914789 is a long-period variable star[1].
Key Facts
- Q88914789's instance of is recorded as long-period variable star[2].
- Q88914789's constellation is recorded as Aquila[3].
- Q88914789's spectral class is recorded as M0[4].
- Q88914789's catalog code is recorded as AAVSO 1936+11[5].
- Q88914789's catalog code is recorded as AG+11 2322[6].
- Q88914789's catalog code is recorded as AN 431.1928[7].
- Q88914789's catalog code is recorded as CSI+11-19387[8].
- Q88914789's catalog code is recorded as GSC 01065-03128[9].
- Q88914789's catalog code is recorded as HD 355662[10].
- Q88914789's catalog code is recorded as IRAS 19387+1141[11].
- Q88914789's catalog code is recorded as PPM 136770[12].
- Q88914789's catalog code is recorded as TYC 1065-3128-1[13].
- Q88914789's catalog code is recorded as 2MASS J19410710+1148502[14].
- Q88914789's catalog code is recorded as Gaia DR1 4303182194055984128[15].
- Q88914789's catalog code is recorded as Gaia DR2 4303182198382193280[16].
- Q88914789's catalog code is recorded as MS Aql[17].
- Q88914789's type of variable star is recorded as slow irregular variables of late spectral types[18].
- Q88914789's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.43'}[19].
- Q88914789's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.749'}[20].
- Q88914789's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.894'}[21].
- Q88914789's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.528'}[22].
- Q88914789's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.67'}[23].
- Q88914789's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6007'}[24].
- Q88914789's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0093'}[25].
- Q88914789's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-15.94'}[26].
Body
Definition and Type
Q88914789's instance of is recorded as long-period variable star[2].