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Warm Winds in the Seyfert 1 Galaxy NGC 5548
Published online by Cambridge University Press: 26 May 2016
Abstract
We present the results of a recent long XMM-Newton and Chandra observation on the Seyfert 1 galaxy NGC 5548. This galaxy has a warm absorber with a wide range of ionization stages. The detection of O VI in both the UV and X-rays allows for a direct comparison of the measured column density in both wavelength bands. We also comment on the detection of O V, and its newly measured wavelength.
- Type
- Part 3. Ejection and Outflow
- Information
- Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 356 - 357
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
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