Q60225706
galaxy
Press Enter · cited answer in seconds
0 sources
Q60225706
Summary
Q60225706 is a lenticular galaxy[1].
Key Facts
- Q60225706's instance of is recorded as lenticular galaxy[2].
- Q60225706's instance of is recorded as low-ionization nuclear emission-line region[3].
- Q60225706's galaxy morphological type is recorded as -3[4].
- Q60225706 is part of Q67623386[5].
- Q60225706 is part of Q67625405[6].
- Q60225706 is part of Q67791253[7].
- Q60225706's catalog code is recorded as PGC 32659[8].
- Q60225706's catalog code is recorded as UGC 5991[9].
- Q60225706's catalog code is recorded as LEDA 32659[10].
- Q60225706's catalog code is recorded as 2MASX J10524765+4936454[11].
- Q60225706's catalog code is recorded as NPM1G +49.0180[12].
- Q60225706's catalog code is recorded as SDSS J105247.63+493645.2[13].
- Q60225706's catalog code is recorded as UZC J105247.7+493645[14].
- Q60225706's catalog code is recorded as MCG+08-20-036[15].
- Q60225706's catalog code is recorded as Z 241-26[16].
- Q60225706's catalog code is recorded as Z 1049.8+4952[17].
- Q60225706's catalog code is recorded as Gaia DR2 832602263851353344[18].
- Q60225706's redshift is recorded as {'unit': '1', 'amount': '+0.02262'}[19].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.1366'}[20].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.618'}[21].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.014'}[22].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.715'}[23].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.7'}[24].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.903'}[25].
- Q60225706's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.135'}[26].
Body
Definition and Type
Recorded instance of include lenticular galaxy[2] and low-ionization nuclear emission-line region[3].
Use and Application
Part of include Q67623386[5], Q67625405[6], and Q67791253[7].