Mrk 231 |
the closest ULIRG, BAL QSO and most luminous IR galaxy in the Local Universe |
Mrk 421, Mrk 501 |
are among the highest known energy sources (Mrk 501 is one of the 5 known TeV sources) |
Mrk 116 (=IZw18) |
the most metal-deficient blue compact dwarf galaxy (BCDG) (most of BCDGs are Mrk and SBS galaxies) |
Mrk 938 |
the first dynamic merger discovered observationally |
Mrk 110 |
intermediate between NLS1 and BLS1 (FWHM=4900 km/s); crucial for understanding differences between BLS1s and NLS1s |
Mrk 6 |
shows variations of spectral lines typical of different types of objects (Sy2 & Sy1); very high column density of H in X-rays |
Mrk 766 |
one of the most important NLS1 galaxies |
Mrk 273 |
a wonderful double-double nuclei galaxy |
Mrk 266 |
has a multiple structure nuclear region |
Mrk 231, Mrk 507 |
2 of 5 known super strongest FeII emitters (FeII λ4570 / Hβ > 2) |
Mrk 530, Mrk 993, Mrk 1018 |
change their spectra from Sy1.9 to Sy1.0 |
|
|
 |
 |