9. B8
The spectral type is determined principally from the ratio of Si II 4128-4130 to He I 4144. The luminosity class is determined from the appearance of the wings of the hydrogen lines.
Star | MKK | a | m | HD | |
Per...... | B8 V | 3:01 | +40°34' | 2.2 | B8 |
Tau...... | B8 III | 3:41 | +23 48 | 3.0 | B5p |
Ori...... | B8 Ia | 5:09 | - 8 19 | 0.3 | B8p |
Tau...... | B8 III | 5:20 | +28 31 | 1.8 | B8 |
CMi..... | B8 V | 7:21 | + 8 29 | 3.1 | B8 |
a Leo...... | B8 V | 10:03 | +12 27 | 1.3 | B8 |
Lib....... | B8 V | 15:11 | - 9 1 | 2.7 | B8 |
High resolution image |
High resolution image |