Péridier Library Abstract Archive
Abstract No. UT 342
Title: Occlusion Effects and the Distribution of Interstellar Cloud Sizes and Masses
Author(s): J. Scalo, A. Lazarian (University of Texas at Austin)
Keywords: clouds, extinction, occlusion
E-Mail: J. Scalo (to request a full copy of this paper)
Preprint: 9508062 Document source or PostScript
Release date: 08/17/95 11:41:49
Comments: 13 pages, 0 figures
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 that selection effects play a major
role in all the surveys. We conclude that a reliable determination of the
"true" size and mass spectra of clouds will require spectral line surveys
with very high signal-to-noise and sufficient resolution and sampling to
cover a larger range of linear sizes, as well as careful attention to
selection effects.