2MASS wide field extinction maps - III. The Taurus, Perseus, and California cloud complexes

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Table 3:

The masses of the Taurus, Perseus, and California dark complexes.
Cloud	Distance	Mass
		Total	A_K > 0.1	A_K > 0.2
Taurus	$150 ~\mbox{ pc}$	$\phantom{0}20~300 ~ { M}_\odot$	$\phantom{0}15~500~ \mbox{ M}_\odot$	$\phantom{0}8~300~ { M}_\odot$
Perseus	$240 ~\mbox{ pc}$	$\phantom{0}27~000~ { M}_\odot$	$\phantom{0}19~600 ~ { M}_\odot$	$\phantom{0}9~300~ { M}_\odot$
California	$450 ~\mbox{ pc}$	$132~000 ~ { M}_\odot$	$100~000 ~ { M}_\odot$	$43~900 ~ { M}_\odot$

Notes. The small differences with respect to the results reported in Table 1 by Lada et al. (2009) are due to the different resolution of the extinction maps used.

Source LaTeX | All tables | In the text

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