4. B0.5
The blend at 
 4640-4650 is strongest at the red
edge and is 
intermediate in appearance  between B0 and B1. Si III 4552  is
approximately equal to Si IV 4089. Luminosity differences are
shown by 
the lines of O II near H
. They are very strong in the spectrum of the
supergiant 
 Cas. The line
ratios used for luminosity classification 
are 
 3995:
 4009,
 4119:
 4144,
 4349:
 4387, and
 4416:
 4387.
| Star | MKK | a |    | m | HD | 
  CAs....   | B0.5 I | 0:27 | +62° 23' | 4.2 | B0 | 
  Per......   | B0.5 III | 3:51 | +39 43 | 3.0 | B1 | 
| 139 Tau.. | B0.5 II | 5:51 | +25 56 | 4.9 | B2 | 
  Sco.....
  | B0.5 IV | 15:59 | -19 32 | 2.9 | B1 | 
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