Mass outflow in the seyfert 1 galaxy NGC 5548

D. M. Crenshaw, S. B. Kraemer, H. R. Schmitt, J. S. Kaastra, N. Arav, Jack Gabel, K. T. Korista

Research output: Contribution to journalArticle

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Abstract

We present a study of the intrinsic UV absorption and emission lines in an historically low-state spectrum of the Seyfert 1 galaxy NGC 5548, which we obtained in 2004 February at high spatial and spectral resolution with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. We isolate a component of emission with a width of 680 km s-1 that arises from an "intermediate-line region" (ILR), similar to that we discovered in NGC 4151, at a distance of 1 pc from the central continuum source. From a detailed analysis of the five intrinsic absorption components in NGC 5548 and their behavior over a span of eight years, we present evidence that most of the UV absorbers only partially cover the ILR and do not cover an extended region of UV continuum emission, most likely from hot stars in the circumnuclear region. We also find that four of the UV absorbers are at much greater distances (greater than 70 pc) than the ILR, and none have sufficient NV or CIV column densities to be the ILR in absorption. At least a portion of the UV absorption component 3, at a radial velocity of -530 km s-1, is likely responsible for most of the X-ray absorption, at a distance less than 7 pc from the central source. The fact that we see the ILR in absorption in NGC 4151 and not in NGC 5548 suggests that the ILR is located at a relatively large polar angle (45°) with respect to the narrow-line region outflow axis.

Original languageEnglish
Pages (from-to)281-292
Number of pages12
JournalAstrophysical Journal
Volume698
Issue number1
DOIs
StatePublished - 2009

Fingerprint

outflow
galaxies
absorbers
continuums
hot stars
Hubble Space Telescope
spectral resolution
radial velocity
spectrographs
spatial resolution
telescopes
high resolution
x rays

All Science Journal Classification (ASJC) codes

  • Space and Planetary Science
  • Astronomy and Astrophysics
  • Nuclear and High Energy Physics

Cite this

Crenshaw, D. M., Kraemer, S. B., Schmitt, H. R., Kaastra, J. S., Arav, N., Gabel, J., & Korista, K. T. (2009). Mass outflow in the seyfert 1 galaxy NGC 5548. Astrophysical Journal, 698(1), 281-292. https://doi.org/10.1088/0004-637X/698/1/281

Mass outflow in the seyfert 1 galaxy NGC 5548. / Crenshaw, D. M.; Kraemer, S. B.; Schmitt, H. R.; Kaastra, J. S.; Arav, N.; Gabel, Jack; Korista, K. T.

In: Astrophysical Journal, Vol. 698, No. 1, 2009, p. 281-292.

Research output: Contribution to journalArticle

Crenshaw, DM, Kraemer, SB, Schmitt, HR, Kaastra, JS, Arav, N, Gabel, J & Korista, KT 2009, 'Mass outflow in the seyfert 1 galaxy NGC 5548', Astrophysical Journal, vol. 698, no. 1, pp. 281-292. https://doi.org/10.1088/0004-637X/698/1/281
Crenshaw DM, Kraemer SB, Schmitt HR, Kaastra JS, Arav N, Gabel J et al. Mass outflow in the seyfert 1 galaxy NGC 5548. Astrophysical Journal. 2009;698(1):281-292. https://doi.org/10.1088/0004-637X/698/1/281
Crenshaw, D. M. ; Kraemer, S. B. ; Schmitt, H. R. ; Kaastra, J. S. ; Arav, N. ; Gabel, Jack ; Korista, K. T. / Mass outflow in the seyfert 1 galaxy NGC 5548. In: Astrophysical Journal. 2009 ; Vol. 698, No. 1. pp. 281-292.
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