articleThe Astrophysical JournalAug 20, 2003BRONZE OA

A Quantitative Comparison of the Small Magellanic Cloud, Large Magellanic Cloud, and Milky Way Ultraviolet to Near‐Infrared Extinction Curves

KDKarl D. GordonGCGeoffrey C. ClaytonKAK. A. MisseltAUArlo U. LandoltMJMichael J. Wolff

University of Arizona · Louisiana State University · +1 more institution

Indexed inarxivcrossrefdoaj

Abstract

We present an exhaustive, quantitative comparison of all of the known extinction curves in the Small and Large Magellanic Clouds (SMC and LMC) with our understanding of the general behavior of Milky Way extinction curves. The R_V dependent CCM relationship and the sample of extinction curves used to derive this relationship is used to describe the general behavior of Milky Way extinction curves. The ultraviolet portion of the SMC and LMC extinction curves are derived from archival IUE data, except for one new SMC extinction curve which was measured using HST/STIS observations. The optical extinction curves are derived from new (for the SMC) and literature UBVRI photometry (for the LMC). The near-infrared…

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Authors

5
  • KD
    Karl D. GordonCorresponding

    University of Arizona

  • GC
    Geoffrey C. Clayton

    Louisiana State University

  • KA
    K. A. Misselt

    University of Arizona

  • AU
    Arlo U. Landolt

    Louisiana State University

  • MJ
    Michael J. Wolff

    Space Science Institute

Topics & keywords

Keywords
  • Milky Way
  • Extinction (optical mineralogy)
  • Photometry (optics)
  • Small Magellanic Cloud
  • Light curve
  • Large Magellanic Cloud
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