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 |
![]() | B0.5 I | 0:27 | +62° 23' | 4.2 | B0 |
![]() | B0.5 III | 3:51 | +39 43 | 3.0 | B1 |
139 Tau.. | B0.5 II | 5:51 | +25 56 | 4.9 | B2 |
![]() | B0.5 IV | 15:59 | -19 32 | 2.9 | B1 |
![]() |
High resolution image |