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AbstractAbstract
[en] Results are presented from photoelectric scans of the interstellar lambda3384 line of Ti II obtained at a resolution of 3.7 km s-1 for 47 stars. Although the depletion of titanium from the interstellar gas is large ad highly variable, its ratio to the depletion of interstellar calcium is relatively constant; titanium is less depleted than calcium by a factor of about 4. A method for determining approximate electron densities from the Ca II and Ti II colmn densities is applied to 51 interstellar clouds
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Journal Article
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Astrophys. J., Lett; v. 208(2); p. L95-L98
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