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Dust and Stellar Populations in the Large Magellanic Cloud

  • Authors: Dennis Zaritsky

Zaritsky 1999 The Astronomical Journal 118 2824.

  • Provider: AAS Journals

Caption: Fig. 12.

Comparison of the distribution of ﹩A_{V}﹩ values derived for the hot (﹩T_{E}> 12,000﹩ K; thick solid line) and cool (﹩5500< T_{E}< 6500﹩ K; thin solid line) stars. The dashed areas at ﹩A_{V}< 0﹩ indicate the number of stars with ﹩A_{V}=0﹩, where we have set the height of the bin equal to the number of stars with ﹩A_{V}=0.01﹩ and the area to represent the number of stars correctly. The two histograms have been arbitrarily normalized.

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