On the Taurus dust cloud toward 3C 123

Details On the Taurus dust cloud toward 3C 123 On the Taurus dust cloud toward 3C 123

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239..549c&link_type=abstract

Astrophysical Journal, Part 1, vol. 239, July 15, 1980, p. 549-554.

Astronomy and Astrophysics

Astronomy

19

Clouds, Cosmic Dust, Interstellar Matter, Absorption Spectra, Astronomical Models, D Lines, Hydroxyl Emission, Line Spectra, Radio Astronomy, Spatial Distribution

Scientific paper

In the present paper, the results of the Guibert, Elitzur, Nguyen-Q-Rieu (1978) analysis are used as a basis to test and refine the parameters of a model for the cloud toward 3C 123. From the analysis, the Taurus clouds appear to have a sheetlike geometry with an extent more than an order of magnitude greater than the thickness. It might be suggested that a one-dimensional compression occurred in Taurus and that the dense core portion of the cloud has fragmented to create the clumps, one of which is exemplified by Cloud 2.

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