The Shapes of Dense Cores and Bok Globules

Details The Shapes of Dense Cores and Bok Globules The Shapes of Dense Cores and Bok Globules

1996-08-02

arxiv.org/abs/astro-ph/9608014v1

Astronomy and Astrophysics

Astrophysics

26 pages (LaTeX) including 8 postscript figures; to appear in ApJ

Scientific paper

10.1086/178010

The shapes of isolated Bok globules and embedded dense cores of molecular clouds are analyzed using a nonparametric method, under the alternate hypotheses that they are randomly oriented prolate objects or that they are randomly oriented oblate objects. In all cases, the prolate hypothesis gives a better fit to the data. If Bok globules are oblate, they must be very flat; the average axis ratio is b/a = 0.3, and few or no globules can have b/a > 0.7. If Bok globules are prolate, then the mean axis ratio is b/a = 0.5. For most data samples of dense cores, the randomly-oriented oblate hypothesis can be rejected at the 99% confidence level. If the dense cores are prolate, their mean axis ratio is approximately 0.4 to 0.5. Dense cores are significantly different in shape from the clouds in which they are embedded; clouds have flatter apparent shapes, and are inconsistent with a population of randomly oriented axisymmetric objects.

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