Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T09:36:04.249Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 

References

Arav, N., et al. 2003, ApJ, 590, 174.Google Scholar
Behar, E., private communication.Google Scholar
Beiersdorfer, P. 2003, ARA&A, 41, 343.Google Scholar
Crenshaw, D. M., & Kraemer, S. B. 1999, ApJ, 521, 57.Google Scholar
Done, C., Pounds, K. A., Nandra, K., & Fabian, A. C. 1995, MNRAS, 275, 417.Google Scholar
Schmidt, M. & Beiersdorfer, P., private communication.Google Scholar
Steenbrugge, K. C., Kaastra, J. S., de Vries, C. P. & Edelson, R. 2003, A&A, 402, 477.Google Scholar
Steenbrugge, K. C., et al. 2004, in prep.Google Scholar