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相关论文: Temperature Discrepancy with Photoionization Model…

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Different studies have reported the so-called temperature problem of the narrow line region (NLR) of active galactic nuclei (AGNs). Its origin is still an open issue. To properly address its cause, a trustworthy temperature indicator is…

We investigate the discrepancy between oxygen abundance estimations for narrow-line regions (NLRs) of Active Galactic Nuclei (AGNs) type Seyfert 2 derived by using direct estimations of the electron temperature (Te-method) and those derived…

星系天体物理 · 物理学 2020-07-01 O. L. Dors , R. Maiolino , M. V. Cardaci , G. F. Hagele , A. C. Krabbe , E. Perez-Montero , M. Armah

We study the prototypical Seyfert 2 galaxy, Markarian 3, based on imaging and high-resolution spectroscopy observations taken by the Chandra X-ray Observatory. We construct a deconvolved X-ray image, which reveals the S-shaped morphology of…

高能天体物理现象 · 物理学 2017-10-18 Akos Bogdan , Ralph P. Kraft , Daniel A. Evans , Felipe Andrade-Santos , William R. Forman

We present multi-component photoionization models allowing for local density inhomogeneities in the NLR to interpret the emission line spectra of Seyfert 2 galaxies. This approach leads to a successful match of a large set of line…

天体物理学 · 物理学 2016-08-30 Stefanie Komossa , Hartmut Schulz

We study the narrow-line region (NLR) of six Seyfert-1 and six Seyfert-2 galaxies by means of spatially resolved optical spectroscopy and photoionization modelling. From spatially resolved spectral diagnostics, we find a transition between…

天体物理学 · 物理学 2007-05-23 Nicola Bennert , Bruno Jungwiert , Stefanie Komossa , Martin Haas , Rolf Chini , ;

The remarkable similarity between emission spectra of narrow line regions (NLR) in Seyfert Galaxies has long presented a mystery. In photoionization models, this similarity implies that the ionization parameter is nearly always the same,…

天体物理学 · 物理学 2009-11-07 M. A. Dopita , B. A. Groves , R. S. Sutherland , L. Binette , G. Cecil

We have investigated the physical conditions in the narrow-line region (NLR) of M51 using long-slit spectra obtained with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope (HST) and 3.6 cm radio continuum…

天体物理学 · 物理学 2009-11-10 L. D. Bradley , M. E. Kaiser , W. A. Baan

We have compared the optical emission line ratios of type 2 quasars from Zakamska et al. with standard AGN photoionization model predictions, Seyfert 2s, HII galaxies, and narrow line FRII radio galaxies. Moderate to high ionization narrow…

We present a study of the distribution of [O III] $\lambda$5007 and [O II] $\lambda$3727 emission in the Narrow Line Region (NLR) of the Seyfert 1 galaxy NGC 4151. While the NLR of NGC 4151 exhibits an overall structure consistent with the…

天体物理学 · 物理学 2009-11-13 S. B. Kraemer , H. R. Schmitt , D. M. Crenshaw

The presence of an active galactic nucleus (AGN) can strongly affect its host. Due to the copious radiative power of the nucleus, the effects of radiative feedback can be detected over the entire host galaxy and sometimes well into the…

星系天体物理 · 物理学 2018-05-02 Ross Dempsey , Nadia Zakamska

We systematically determine the electron density and electron temperature of active galaxies and star-forming galaxies using spectroscopy from the SDSS DR7, while mainly focusing on the NLRs. Density and temperature are determined through…

宇宙学与河外天体物理 · 物理学 2013-02-18 Zhitai Zhang , Yanchun Liang , François Hammer

The temperature predicted by photoionization models for the Narrow Line Region of Seyfert 2 galaxies is lower than the value inferred from the observed [O III] {\lambda}4363A/{\lambda}5007A line ratio. We explore the possibility of…

星系天体物理 · 物理学 2023-04-12 Luc Binette , Yair Krongold , Sinhue A. R. Haro-Corzo , Andrew Humphrey , Sandy G. Morais

We present spatially resolved long-slit spectroscopy from the Southern African Large Telescope (SALT) to examine the spatial extent of the narrow-line regions (NLRs) of a sample of 8 luminous obscured quasars at 0.10 < z < 0.43. Our results…

宇宙学与河外天体物理 · 物理学 2015-06-16 Kevin N. Hainline , Ryan C. Hickox , Jenny E. Greene , Adam D. Myers , Nadia L. Zakamska

While [OIII] narrow-band imaging is commonly used to measure the size of the narrow-line regions (NLRs) in active galactic nuclei (AGNs), it can be contaminated by emission from surrounding starbursts. Recently, we have shown that long-slit…

天体物理学 · 物理学 2009-11-11 Nicola Bennert , Bruno Jungwiert , Stefanie Komossa , Martin Haas , Rolf Chini

We study the narrow-line region (NLR) of the Seyfert-2 galaxy NGC 1386 by means of long-slit spectroscopy obtained with FORS1 at the VLT. We use the galaxy itself for subtracting the stellar template, applying reddening corrections to fit…

天体物理学 · 物理学 2009-11-11 Nicola Bennert , Bruno Jungwiert , Stefanie Komossa , Martin Haas , Rolf Chini

We consider a model in which the narrow line regions (NLRs) of Seyfert galaxies are photoionized ``in situ'' by fast (300 -- 1,000 km/s), radiative shock waves driven into the interstellar medium of the galaxy by radio jets from the active…

天体物理学 · 物理学 2009-10-31 A. S. Wilson , J. C. Raymond

We derive the nitrogen and oxygen abundances in the Narrow Line Regions (NLRs) of a sample of 38 local ($z \: < \: 0.4$) Seyfert~2 nuclei. For that, we consider narrow optical emission line intensities and direct estimates of the electron…

The ionization mechanism of the low-ionization gas in quiescent red sequence galaxies has been a long-standing puzzle. Direct temperature measurements would put strong constraints on this issue. We carefully selected a sample of quiescent…

星系天体物理 · 物理学 2018-08-15 Renbin Yan

We present a study of reddening and absorption towards the Narrow Line Regions (NLR) in active galactic nuclei (AGN) selected from the Revised Shapley-Ames, 12mu, and Swift/Burst Alert Telescope samples. For the sources in host galaxies…

宇宙学与河外天体物理 · 物理学 2015-05-20 S. B. Kraemer , H. R. Schmitt , D. M. Crenshaw , M. Melendez , T. J. Turner , M. Guainazzi. , R. F. Mushotzky

We have observed the narrow-line regions (NLRs) of the seven brightest radio-quiet PG (or BQS) quasars (z < 0.5) with the Wide Field and Planetary Camera 2 on board the Hubble Space Telescope (HST). Linear-ramp filters were used to image…

天体物理学 · 物理学 2009-11-07 Nicola Bennert , Heino Falcke , Hartmut Schulz , Andrew S. Wilson , Beverley J. Wills
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