The Suzaku observation of the nucleus of the radio-loud active galaxy centaurus a: Constraints on abundances of the accreting material

A. Markowitz, T. Takahashi, S. Watanabe, K. Nakazawa, Y. Fukazawa, M. Kokubun, K. Makishima, H. Awaki, A. Bamba, N. Isobe, Jun Kataoka, G. Madejski, R. Mushotzky, T. Okajima, A. Ptak, J. N. Reeves, Y. Ueda, T. Yamasaki, T. Yaqoob

Research output: Contribution to journalArticle

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Abstract

A Suzaku observation of the nucleus of the radio-loud AGN Centaurus A in 2005 has yielded a broadband spectrum spanning 0.3-250 keV. The net exposure times after screening were 70 ks per X-ray Imaging Spectrometer (XIS) camera, 60.8 ks for the Hard X-ray Detector ( HXD) PIN, and 17.1 ks for the HXD GSO. The hard X-rays are fit by two power laws of the same slope, absorbed by columns of 1.5 and 7 × 1023 cm-2, respectively. The spectrum is consistent with previous suggestions that the power-law components are X-ray emission from the subparsec VLBI jet and from Bondi accretion at the core, but it is also consistent with a partial-covering interpretation. The soft band is dominated by thermal emission from the diffuse plasma and is fit well by a two-temperature VAPEC model, plus a third power-law component to account for scattered nuclear emission, jet emission, and emission from X-ray binaries and other point sources. Narrow fluorescent emission lines from Fe, Si, S, Ar, Ca, and Ni are detected. The Fe Ka line width yields a 200 It-day lower limit on the distance from the black hole to the line-emitting gas. Fe, Ca, and S K-shell absorption edges are detected. Elemental abundances are constrained via absorption edge depths and strengths of the fluorescent and diffuse plasma emission lines. The high metallicity ([Fe/H] = +0.1) of the circumnuclear material suggests that it could not have originated in the relatively metal-poor outer halo unless enrichment by local star formation has occurred. Relative abundances are consistent with enrichment from Type II and Ia supernovae. 2007. The American Astronomical Society. All rights reserved.

Original languageEnglish
Pages (from-to)209-224
Number of pages16
JournalAstrophysical Journal
Volume665
Issue number1 PART 1
DOIs
Publication statusPublished - 2007 Aug 10
Externally publishedYes

Fingerprint

active galaxies
radio galaxies
radio
nuclei
x rays
power law
very long base interferometry
detectors
plasma
imaging spectrometers
thermal emission
very long baseline interferometry
point sources
metallicity
suggestion
supernovae
material
star formation
halos
coverings

Keywords

  • Galaxies: active
  • Galaxies: individual (NGC 5128)
  • X-rays: galaxies

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Markowitz, A., Takahashi, T., Watanabe, S., Nakazawa, K., Fukazawa, Y., Kokubun, M., ... Yaqoob, T. (2007). The Suzaku observation of the nucleus of the radio-loud active galaxy centaurus a: Constraints on abundances of the accreting material. Astrophysical Journal, 665(1 PART 1), 209-224. https://doi.org/10.1086/519271

The Suzaku observation of the nucleus of the radio-loud active galaxy centaurus a : Constraints on abundances of the accreting material. / Markowitz, A.; Takahashi, T.; Watanabe, S.; Nakazawa, K.; Fukazawa, Y.; Kokubun, M.; Makishima, K.; Awaki, H.; Bamba, A.; Isobe, N.; Kataoka, Jun; Madejski, G.; Mushotzky, R.; Okajima, T.; Ptak, A.; Reeves, J. N.; Ueda, Y.; Yamasaki, T.; Yaqoob, T.

In: Astrophysical Journal, Vol. 665, No. 1 PART 1, 10.08.2007, p. 209-224.

Research output: Contribution to journalArticle

Markowitz, A, Takahashi, T, Watanabe, S, Nakazawa, K, Fukazawa, Y, Kokubun, M, Makishima, K, Awaki, H, Bamba, A, Isobe, N, Kataoka, J, Madejski, G, Mushotzky, R, Okajima, T, Ptak, A, Reeves, JN, Ueda, Y, Yamasaki, T & Yaqoob, T 2007, 'The Suzaku observation of the nucleus of the radio-loud active galaxy centaurus a: Constraints on abundances of the accreting material', Astrophysical Journal, vol. 665, no. 1 PART 1, pp. 209-224. https://doi.org/10.1086/519271
Markowitz, A. ; Takahashi, T. ; Watanabe, S. ; Nakazawa, K. ; Fukazawa, Y. ; Kokubun, M. ; Makishima, K. ; Awaki, H. ; Bamba, A. ; Isobe, N. ; Kataoka, Jun ; Madejski, G. ; Mushotzky, R. ; Okajima, T. ; Ptak, A. ; Reeves, J. N. ; Ueda, Y. ; Yamasaki, T. ; Yaqoob, T. / The Suzaku observation of the nucleus of the radio-loud active galaxy centaurus a : Constraints on abundances of the accreting material. In: Astrophysical Journal. 2007 ; Vol. 665, No. 1 PART 1. pp. 209-224.
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abstract = "A Suzaku observation of the nucleus of the radio-loud AGN Centaurus A in 2005 has yielded a broadband spectrum spanning 0.3-250 keV. The net exposure times after screening were 70 ks per X-ray Imaging Spectrometer (XIS) camera, 60.8 ks for the Hard X-ray Detector ( HXD) PIN, and 17.1 ks for the HXD GSO. The hard X-rays are fit by two power laws of the same slope, absorbed by columns of 1.5 and 7 × 1023 cm-2, respectively. The spectrum is consistent with previous suggestions that the power-law components are X-ray emission from the subparsec VLBI jet and from Bondi accretion at the core, but it is also consistent with a partial-covering interpretation. The soft band is dominated by thermal emission from the diffuse plasma and is fit well by a two-temperature VAPEC model, plus a third power-law component to account for scattered nuclear emission, jet emission, and emission from X-ray binaries and other point sources. Narrow fluorescent emission lines from Fe, Si, S, Ar, Ca, and Ni are detected. The Fe Ka line width yields a 200 It-day lower limit on the distance from the black hole to the line-emitting gas. Fe, Ca, and S K-shell absorption edges are detected. Elemental abundances are constrained via absorption edge depths and strengths of the fluorescent and diffuse plasma emission lines. The high metallicity ([Fe/H] = +0.1) of the circumnuclear material suggests that it could not have originated in the relatively metal-poor outer halo unless enrichment by local star formation has occurred. Relative abundances are consistent with enrichment from Type II and Ia supernovae. 2007. The American Astronomical Society. All rights reserved.",
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AU - Fukazawa, Y.

AU - Kokubun, M.

AU - Makishima, K.

AU - Awaki, H.

AU - Bamba, A.

AU - Isobe, N.

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