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Warm Winds in the Seyfert 1 Galaxy NGC 5548

Published online by Cambridge University Press:  26 May 2016

K. C. Steenbrugge  and
J. S. Kaastra
K. C. Steenbrugge
Affiliation:
SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
J. S. Kaastra
Affiliation:
SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands

Abstract

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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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