Star formation efficiency e versus
cloud mass Mc determined for a full sample of 39
clouds associated with 83 HII regions.
The cross shows typical errors of 0.3 in log10Mc
and 0.4 in log10e. The
diagonal dashed line shows the efficiency a cloud would have if
associated with an HII region of luminosity
Lmin = 400 Jy kpc2. The data are incomplete
below this line. The vertical dashed line shows the molecular
cloud survey completeness boundary at Mc = 4 x 105
solar masses.
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