X-ray astronomy of stellar coronae

@article{Gdel2004XrayAO,
  title={X-ray astronomy of stellar coronae},
  author={M. G{\"u}del},
  journal={The Astronomy and Astrophysics Review},
  year={2004},
  volume={12},
  pages={71-237}
}
  • M. Güdel
  • Published 2004
  • Physics
  • The Astronomy and Astrophysics Review
Abstract.X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally attributed to the presence of a magnetic corona that contains plasma at temperatures exceeding 1 million K. Coronae are ubiquitous among these stars, yet many fundamental mechanisms operating in their magnetic fields still elude an interpretation through a detailed physical description. Stellar X-ray astronomy is therefore contributing toward a deeper understanding of the generation of magnetic… Expand
X-ray observations of central stars of planetary nebulae and their winds
  • M. Guerrero
  • Physics
  • Proceedings of the International Astronomical Union
  • 2011
The 6.7 keV Line Emission from the Stellar Flare of Algol
Ionization and heating by X-rays and cosmic rays
...
1
2
3
4
5
...

References

SHOWING 1-4 OF 4 REFERENCES