Fig 15 - uploaded by Charlène Lefèvre
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Summary of the derived maximum grain size ranges for the modeled sources. The black bar gives the range where R theo is in the FWHM range of R obs , and the blue (green) bar shows the range for the model maximum coreshine to be within the observed maximum coreshine range at 3.6 (4.5) µm, respectively. For L1439, we also give size ranges for a model that includes a local radiation field. Light green boxes indicate ranges of agreement.
Source publication
Recently discovered scattered light from molecular cloud cores in the
wavelength range 3-5 {\mu}m (called "coreshine") seems to indicate the presence
of grains with sizes above 0.5 {\mu}m. We aim to analyze 3.6 and 4.5 {\mu}m
coreshine from molecular cloud cores to probe the largest grains in the size
distribution. We analyzed dedicated deep Cycle...
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