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Numerical values showing gel band strength were used to calculate the percentage of change in the expression of P5CS.
Our calculations have shown variations in the band strength, but there were no significant changes in the profile.
This statement also applies to most of the C60 sources, and thus additional complexity can be introduced into the discussion of band strength ratios in the next section.
The calculations, including those for silicate, show a decrease in the band strength but the changes in the stretching mode profile of CO ice are not significant.
The difference in the strength of absorption bands for the stretching vibration of N H before and after the phosphonation could be observed, with the phosphonated polymer yielding lower band strength.
Adding S11 and L15 data (unique to the AKARI survey) ensures additional new features and can be essential for the estimation of the silicate band strength in mass-losing stars (Kato et al., 2009; Onaka et al., 2009).
Similar(49)
The relative band strengths do not vary appreciably in this range.
Motivated by detections of glycolaldehyde and ethylene glycol in the interstellar medium and, for ethylene glycol, in comet Hale-Bopp, we report the low-temperature mid-IR spectra of these two molecules, including selected band strengths and positions.
Further studies of the UIR bands in different environments show that the band strengths are linearly proportional to the intensity of incident radiation field as long as the incident intensity is in the range from unity to 100 times the solar vicinity value.
C60 band strengths normalized to that of the 18.9 μ m feature.
The theoretical band strengths are remarkably inconsistent with the experimental values.
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