Warm Dust and Spatially Variable Polycyclic Aromatic Hydrocarbon Emission in the Dwarf Starburst Galaxy NGC 1705

@article{Cannon2006WarmDA,
  title={Warm Dust and Spatially Variable Polycyclic Aromatic Hydrocarbon Emission in the Dwarf Starburst Galaxy NGC 1705},
  author={J. Cannon and J. Smith and F. Walter and G. Bendo and D. Calzetti and D. Dale and B. Draine and C. Engelbracht and K. Gordon and G. Helou and R. Kennicutt and Jr. and C. Leitherer and L. Armus and B. Buckalew and D. Hollenbach and T. Jarrett and Aigen Li and M. Meyer and E. Murphy and M. Regan and G. Rieke and M. Rieke and H. Roussel and K. Sheth and M. Thornley},
  journal={The Astrophysical Journal},
  year={2006},
  volume={647},
  pages={293-302}
}
We present Spitzer observations of the nearby dwarf starburst galaxy NGC 1705 obtained as part of the Spitzer Infrared Nearby Galaxies Survey. The galaxy morphology is very different shortward and longward of ~5 μm: optical and short-wavelength IRAC imaging shows an underlying red stellar population, with the central super star cluster (SSC) dominating the luminosity; longer wavelength IRAC and MIPS imaging reveals warm dust emission arising from two off-nuclear regions that are offset by ~250… Expand
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