The correlations can be expressed in the form

$m_{T} = C - K \log d,$ (1)

where K is constant from type to type, but C varies progressively

throughout the sequence. The value of K cannot be accurately

determined from the scattered data for any particular type, but,

within the limits of uncertainty, it approximates the round number 5.0,

the value which is represented by the lines in Figures 2–5.

When K is known, the value of C can be computed from the mean magnitude

and the logarithm of the diameter for each type. This amounts to

reading from the curves the magnitudes corresponding to a diameter

of one minute of arc, but avoids the uncertainty of establishing the

curves where the data are limited.

TABLE IV

Irregular Nebulae

==========+===========+=========

N.G.C. | m_{T} | log d

----------+-----------+---------

2968 | 12.6 | +0.08

3034* | 9.0 | .85

3077 | 11.4 | .48

3729 | 11.8 | .17

4214* | 11.3 | .90

4449* | 9.5 | .65

4618 | 12.3 | +0.40

4656§ | 11.5 | +1.30

4753 | 11.4 | +0.43

5144 | 12.8 | – .30

5363 | 11.1 | +0.20

----------+-----------+---------

Mean | 11.34 | +0.469

----------+-----------+---------

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