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相关论文: The evidence for jet-cloud interactions in a sampl…

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We present results of Gemini spectroscopy and Hubble Space Telescope imaging of the 3C~381 radio galaxy. Possible ionising mechanisms for the Extended Emission-Line Region were studied through state-of-the-art diagnostic analysis employing…

星系天体物理 · 物理学 2015-06-12 V. Reynaldi , C. Feinstein

An analysis of the kinematics and ionisation state of the emission line gas of a sample of 14 3CR radio galaxies with redshifts z~1 is carried out. The data used for these studies, deep long--slit spectroscopic exposures from the WHT, are…

天体物理学 · 物理学 2009-10-31 P. N. Best , H. J. A. R"ottgering , M. S. Longair

Integral-field spectroscopic observations are presented for three powerful radio galaxies, namely 3C277.3 (Coma A; z=0.0857), 3C171 (z=0.2384) and 3C265 (z=0.811), which are known to be undergoing jet-cloud interactions. The morphology,…

天体物理学 · 物理学 2009-11-07 C. Solorzano-Inarrea , C. N. Tadhunter

We present deep, narrow-band and continuum images of the powerful z=0.811 radio galaxy 3C265, taken with the TTF on the WHT, together with detailed long-slit spectroscopic observations along the axis defined by the UV/optical emission…

天体物理学 · 物理学 2011-03-10 C. Solorzano-Inarrea , C. Tadhunter , J. Bland-Hawthorn

We present new Gemini spectroscopical data of the Extended Emission-Line Region of 3C~305 radio galaxy in order to achieve the final answer of the long-standing question about the ionizing mechanism. The spectra show strong kinematic…

宇宙学与河外天体物理 · 物理学 2015-06-16 Victoria Reynaldi , Carlos Feinstein

This paper is the second in a series in which we present intermediate-resolution spectra for a complete sample of 14 compact radio sources, taken with the aim of investigating the impact of the nuclear activity on the cirumnuclear…

宇宙学与河外天体物理 · 物理学 2010-11-02 J. Holt , C. N. Tadhunter , R. Morganti

We present spatially resolved maps of morphology, kinematics, and energetics of warm ionized gas in six powerful radio galaxies at z=3.5-4, using JWST/NIRSpec IFU to quantify jet-driven feedback in the early universe. All sources exhibit…

星系天体物理 · 物理学 2025-08-12 Namrata Roy , Timothy Heckman , Alaina Henry

In this article I review the dominant physical mechanisms in the extended emission line regions (EELR) of powerful radio galaxies at low redshifts and, in particular, the balance between jet-induced shocks and AGN photoionization. I…

天体物理学 · 物理学 2007-05-23 Clive N. Tadhunter

We report the detection of extended warm ionized gas in two powerful high-redshift radio galaxies, NVSS J210626-314003 at z=2.10 and TXS 2353-003 at z=1.49, that does not appear to be associated with the radio jets. This is contrary to what…

The high redshift radio galaxy 4C41.17 consists of a powerful radio source in which previous work has shown that there is strong evidence for jet-induced star formation along the radio axis. We argue that nuclear photoionization is not…

We present an investigation into the nature of the jet-gas interactions in a sample of 10 radio galaxies at 2.3<z<2.9 using deep spectroscopy of the UV line and continuum emission obtained at Keck II and the Very Large Telescope.…

天体物理学 · 物理学 2009-11-11 A. Humphrey , M. Villar-Martin , R. Fosbury , J. Vernet , S. di Serego Alighieri

We present optical and radio images, and long-slit spectra of the radio galaxy PKS 1932-464 (z=0.230). Our main goal is to determine whether the observed properties of the extended emission line nebulosity in this object show evidence for…

天体物理学 · 物理学 2007-05-23 M. Villar-Martin , C. N. Tadhunter , R. Morganti , N. E. Clark , N. Killeen , D. Axon

We present UV rest frame spectra of 3 powerful narrow line radio galaxies and the hyperluminous type 2 active galaxy SMM02399-0136, all at high redshift (z>2). We find high velocities (FWHM>1000, km/s) in the extended gas of all objects. A…

天体物理学 · 物理学 2007-05-23 M. Villar-Martin , L. Binette , R. A. E. Fosbury

Deep, narrow-band Halpha observations taken with the TAURUS Tunable Filter (TTF) on the 4.2m WHT telescope are presented for two nearby radio galaxies with strong jet-cloud interactions. Although the brightest emission line components are…

天体物理学 · 物理学 2009-10-31 C. N. Tadhunter , M. Villar-Martin , R. Morganti , J. Bland-Hawthorn , D. Axon

We present Hubble Space Telescope Imaging Spectrograph long-slit spectroscopy of the emission line nebulae in the compact steep spectrum radio sources 3C 67, 3C 277.1, and 3C 303.1. We derive BPT (Baldwin- Philips-Terlevich; Baldwin et al.…

We investigate the ionization state of the Extended Emission-Line Regions (EELRs) around two compact steep-spectrum (CSS) radio galaxies, 3C~268.3 and 3C~303.1, in order to identify the contribution of photoionization and shock-ionization.…

星系天体物理 · 物理学 2015-12-02 V. Reynaldi , C. Feinstein

Deep long-slit spectroscopic data are presented for a sample of 14 3CR radio galaxies at redshift z ~ 1, previously studied in detail using the Hubble Space Telescope, the Very Large Array, and UKIRT. Analysis of the [OII] 3727 emission…

天体物理学 · 物理学 2009-10-31 P. N. Best , H. J. A. R"ottgering , M. S. Longair

We have compiled a sample of 165 radio galaxies from the literature to study the properties of the extended emission line regions and their interaction with the radio source over a large range of redshift 0<z<5.2. For each source, we have…

天体物理学 · 物理学 2007-05-23 Carlos De Breuck , Huub Rottgering , George Miley , Wil van Breugel , Philip Best

We present integral field spectroscopy of a small sample of radio-loud quasars at intermediate redshift (0.26<z<0.60), most of which are associated with large radio sources. All have oxygen line emission extended over tens of kiloparcsecs,…

天体物理学 · 物理学 2009-10-31 C. S. Crawford , C. Vanderriest

We have used high resolution longslit spectroscopy to investigate the ionized gas in the active galaxy IRAS 04210+0400 and its association with the radio structure. We suggest that two of the ionized components are associated with the…

天体物理学 · 物理学 2015-06-24 A. J. Holloway , W. Steffen , A. Pedlar , D. J. Axon , J. E. Dyson , J. Meaburn , C. N. Tadhunter
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