5.5. The K-System
This is the most numerous group of all and comprises 23 galaxies having a great diversity in appearance. Their spectra, however, indicate that the principal contribution to the total luminosity in the blue-violet region is probably from K-type giant stars. The K-systems are listed in Table V, and they all have one property in common: the major part of the luminosity originates in a brilliant, amorphous central region.
NGC | Hubble | NGC | Hubble | NGC | Hubble |
224 (M 31) | Sb | 4111 | S0 | 4649 (M 60) | E2 |
1398 | SBb | 4216 | Sb | 4699 | Sb |
2841 | Sb | 4260 | SBa | 4762 | Sa |
2950 | SB0 | 4486 (M 87) | E0 | 5308 | S0 |
3031 (M 81) | Sb | 4565 | Sb | 5363 | Irr |
3115 | E7 | 4594 | Sb | 5473 | SB0 |
3990 | S0 | 4636 | E0 | 5850 | SBb |
3998 | S0 | 4643 | SB0 |
The forms of the K-systems fall into several well-defined groups: (1) the great Sb and Sa spiral systems; (2) barred spirals of strong central concentration of light; (3) the giant elliptical systems; (4) "dustless" systems similar in figure to the Sa-Sb spirals; (5) nondescript systems.