Q88627417
emission-line star in the constellation Mensa
Press Enter · cited answer in seconds
0 sources
Q88627417
Summary
Q88627417 is an emission-line star[1].
Key Facts
- Q88627417's instance of is recorded as emission-line star[2].
- Q88627417's constellation is recorded as Mensa[3].
- Q88627417's spectral class is recorded as B0III[e][4].
- Q88627417's catalog code is recorded as OGLE LMC137.1 9867[5].
- Q88627417's catalog code is recorded as OGLE LMC530.11.007532[6].
- Q88627417's catalog code is recorded as GSC 09165-00926[7].
- Q88627417's catalog code is recorded as 2MASS J04532543-7035395[8].
- Q88627417's catalog code is recorded as SK -70 10[9].
- Q88627417's catalog code is recorded as [M2002] LMC 16948[10].
- Q88627417's catalog code is recorded as OGLE LMC-ECL-2253[11].
- Q88627417's catalog code is recorded as [GC2009] J045325.51-703541.2[12].
- Q88627417's catalog code is recorded as [WSI2008] 80[13].
- Q88627417's catalog code is recorded as SSTISAGE1C J045325.57-703541.2[14].
- Q88627417's catalog code is recorded as [RP2006] 1671[15].
- Q88627417's catalog code is recorded as UCAC4 098-005101[16].
- Q88627417's catalog code is recorded as [H2013] LMCe 68[17].
- Q88627417's catalog code is recorded as Gaia DR2 4654738633163743232[18].
- Q88627417's type of variable star is recorded as eclipsing binary star[19].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.896'}[20].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.775'}[21].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.824'}[22].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.770'}[23].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2'}[24].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.500'}[25].
- Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.915'}[26].
Body
Definition and Type
Q88627417's instance of is recorded as emission-line star[2].