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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. 1.

Stellar density plot (for stars with ﹩V< 21﹩) for the region in the LMC with reduced photometry from the Magellanic Cloud Photometric Survey. The central coordinates are roughly ﹩\alpha =5^{\mathrm{h}\,}20^{\mathrm{m}\,}﹩ and ﹩\delta =-66^{\circ }48^{\prime }﹩, and the image is ﹩\sim 4^{\circ }﹩ wide by 2﹩\fdg﹩7 tall, with north at the top and east to the left. Each "pixel" in this plot corresponds to 21﹩\arcsec﹩.

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