Q74105248
long-period variable star in the constellation Cygnus
Press Enter · cited answer in seconds
0 sources
Q74105248
Summary
Q74105248 is a long-period variable star[1].
Key Facts
- Q74105248's instance of is recorded as long-period variable star[2].
- Q74105248's instance of is recorded as infrared source[3].
- Q74105248's instance of is recorded as near-infrared source[4].
- Q74105248's constellation is recorded as Cygnus[5].
- Q74105248's spectral class is recorded as M[6].
- Q74105248's catalog code is recorded as AG+45 1863[7].
- Q74105248's catalog code is recorded as BD+45 3503[8].
- Q74105248's catalog code is recorded as CSV 5402[9].
- Q74105248's catalog code is recorded as GSC 03589-07719[10].
- Q74105248's catalog code is recorded as IRAS 21194+4537[11].
- Q74105248's catalog code is recorded as PPM 61327[12].
- Q74105248's catalog code is recorded as 2MASS J21211873+4551243[13].
- Q74105248's catalog code is recorded as Gaia DR1 1972295642847914368[14].
- Q74105248's catalog code is recorded as Gaia DR2 1972295642847914368[15].
- Q74105248's catalog code is recorded as V1335 Cyg[16].
- Q74105248's catalog code is recorded as TYC 3589-7719-1[17].
- Q74105248's catalog code is recorded as TIC 138870746[18].
- Q74105248's catalog code is recorded as Gaia DR3 1972295642847914368[19].
- Q74105248's type of variable star is recorded as slow irregular variables of late spectral types[20].
- Q74105248's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.85'}[21].
- Q74105248's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.800'}[22].
- Q74105248's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.905'}[23].
- Q74105248's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.660'}[24].
- Q74105248's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.62'}[25].
- Q74105248's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.685637'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].