Magellanic Cloud-Type Interstellar Dust along Low-Density Sight Lines in the Galaxy

@article{Clayton2000MagellanicCI,
  title={Magellanic Cloud-Type Interstellar Dust along Low-Density Sight Lines in the Galaxy},
  author={Geoffrey C. Clayton and Karl D. Gordon and Michael J. Wolff},
  journal={Astrophysical Journal Supplement Series},
  year={2000},
  volume={129},
  pages={147-157}
}
We have studied the UV extinction properties along 30 Galactic sight lines using data from the International Ultraviolet Explorer archive that have never been previously examined. These distant (d > 1 kpc) sight lines were selected to investigate the distribution and physical conditions of gas located in low-density regions of the Galactic disk and halo. The average densities along these sight lines are extremely low. It is likely that they are dominated by the warm intercloud medium and have… 

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