Fig. 6
Correlation plots between a) monochromatic luminosities at 12 m and
source luminosity; b) monochromatic luminosities at 12 m and maser
component of CH3OH emission line; c) masses of HMPOs and the
thermal component of CH3OH emission lines; d) the thermal
and the maser component of CH3OH emission lines; e) the
maser-to-thermal emission ratio and the maser emission; f) the
molecular abundances of HDO and H
O. Sources of our sample are labelled with numbers (1
to 10), sources studied by van der Tak et al.
(2006) are labelled with letters (a to h). Solid line: best linear fit
obtained with a least squares method.
(a)
(b)
(c)
(d)
(e)
(f)
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