The Galactic WN stars. Spectral analyses with line-blanketed model atmospheres versus stellar evolut

@article{Hamann2006TheGW,
  title={The Galactic WN stars. Spectral analyses with line-blanketed model atmospheres versus stellar evolut},
  author={W. Hamann and G. Graefener and A. Liermann},
  journal={Astronomy and Astrophysics},
  year={2006}
}
An infrared light-receiving device includes an optical absorption layer disposed on a principal surface of a substrate and an optical filter disposed on the optical absorption layer, the optical filter including first, second, and third semiconductor regions that are arranged in that order in a direction from the optical absorption layer to the optical filter, each of the first, second, and third semiconductor regions including an n-type InGaAs layer. The optical absorption layer includes a… Expand
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References

SHOWING 1-10 OF 59 REFERENCES
The Treatment of Non-LTE Line Blanketing in Spherically Expanding Outflows
Grids of model spectra for WN stars, ready for use
Correcting for the Effects of Interstellar Extinction
NGC 6611: a cluster caught in the act
The V Sagittae Stars
...
1
2
3
4
5
...