Radial dust density profiles in small molecular clouds

Details Radial dust density profiles in small molecular clouds Radial dust density profiles in small molecular clouds

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...381..474y&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 381, Nov. 10, 1991, p. 474-483. Research supported by Gulbenkian Foundation

Astronomy and Astrophysics

Astronomy

27

Cosmic Dust, Infrared Sources (Astronomy), Interstellar Matter, Molecular Clouds, Grains, Infrared Astronomy Satellite, Nebulae

Scientific paper

A new method for determining the radial volume dust density profiles of dark clouds is presented. This method was applied to coadded IRAS data of 12 small molecular clouds (Bok globules). Raw 60- and 100-micron images were used to generate median filtered backgrounds to be subtracted from the original images. From the resulting differenced images, dust temperature and dust optical depth maps were generated using a single-temperature blackbody model and a dust emissivity proportional to lambda exp -1. These clouds were resolved at the longest IRAS wavelengths and exhibit both regular shapes and structural simplicity. To extract radial dust volume density power laws of the form n(r) varies as r exp -gamma, a collection of dust optical depth contour levels was fitted with ellipses, and the slope of the run of log (column density) versus log (impact parameter) was determined. Modeling enabled determining a relation between the column density power law and the volume density power law for finite-sized clouds. The volume indices gamma were found to be in the range 1 to 5/2, in agreement with previous studies of the gas density. The present rather soft dust indices do not support the hypothesis of grain settlement into the cores of these clouds.

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