Dust-corrected surface photometry of M 31 from Spitzer far-infrared observations

@article{Tempel2010DustcorrectedSP,
  title={Dust-corrected surface photometry of M 31 from Spitzer far-infrared observations},
  author={E. Tempel and A. Tamm and P. Tenjes},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={509}
}
Aims. We create a model for recovering the intrinsic, absorption-corrected surface brightness distribution of a galaxy and apply the model to the nearby galaxy M 31. Methods. We constructed a galactic model as a superposition of axially symmetric stellar components and a dust disc to analyse the intrinsic absorption effects. Dust column density is assumed to be proportional to the far-infrared flux of the galaxy. Along each line of sight, the observed far-infrared spectral energy distribution… Expand
SDSS surface photometry of M 31 with absorption corrections
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Relating dust, gas, and the rate of star formation in M 31
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