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Occlusion Effects and the Distribution of Interstellar Cloud Sizes and Masses
OCCLUSION EFFECTS AND THE DISTRIBUTION OF
INTERSTELLAR CLOUD SIZES AND MASSES
John Scalo and A. Lazarian
Astronomy Department, University of Texas, Austin, TX 78712-1083
5
9 Received ; accepted
9
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u Submitted to the Astrophysical Journal
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– 2 –
ABSTRACT
The frequency distributions of sizes of “clouds” and “clumps” within clouds
are significantly flatter for extinction surveys than for CO spectral line surveys,
even for comparable size ranges. A possible explanation is the blocking of
extinction clouds by larger foreground clouds (occlusion), which should not
affect spectral line surveys much because clouds are resolved in velocity space
along a given line of sight. We present a simple derivation of the relation
between the true and occluded size distributions, assuming clouds are uniformly
distributed in space or the distance to a cloud comples is much greater than the
size of the complex. Because the occlusion is dominated by the largest clouds,
we find that occlusion does not affect the measured size distribution except for
sizes comparable to the largest size, implying that occlusion is not responsible
for the discrepancy if the range in sizes of the samples is large. However, we find
that the range in sizes for many of the published observed samples is actually
quite small, which suggests that occlusion does affect the extinction sample
and/or that the discrepancy could arise from the different operational definitions
and selection effects involved in the two samples. Size and mass spectra from
an IRAS survey (Wood et al. 1994) suggest th
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