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During galaxy merger events, the supermassive black holes in the center of the galaxies may form a pair of active galactic nuclei (AGN) with kpc-scale or even pc-scale separation. Recently, optical observations revealed a promising dual AGN…

星系天体物理 · 物理学 2021-12-22 Patrik Milán Veres , Krisztina É. Gabányi , Sándor Frey , Zsolt Paragi , Emma Kun , Tao An

The knowledge of the physical conditions occurring in the relativistic jet of radio-loud active galactic nuclei (AGNs) is important to understand the mechanisms at the basis of their multiband emission. From parsec-scale radio observations…

宇宙学与河外天体物理 · 物理学 2010-11-29 M. Orienti , G. Giovannini , D. Dallacasa , M. Giroletti , T. Venturi , F. D'Ammando , S. Vercellone , M. Tavani

Perhaps as many as 10% of high redshift radio galaxy (HzRG; z > 2) candidates that are selected using an Ultra Steep radio Spectrum (USS) criterion fail to show optical emission (continuum, lines) in deep Keck exposures. Their parent…

Updates are provided on several issues related to Unified Models. A new HST spectrum of Cygnus A confirms the broad MgII emission line, and suggests a very large velocity width as seen in the polarized optical lines. Statistics of the 3CR…

天体物理学 · 物理学 2007-05-23 Robert Antonucci

We report the discovery of a radio quiet type 2 quasar (SDSS J165315.06+234943.0 nicknamed the "Beetle" at z=0.103) with unambiguous evidence for active galactic nucleus (AGN) radio induced feedback acting across a total extension of ~46…

The radio properties of 11 obscured `radio-intermediate' quasars at redshifts z>~2 have been investigated using the European Very-Long-Baseline-Interferometry Network (EVN) at 1.66 GHz. A sensitivity of ~25 micro Jy per 14x17 mas2 beam was…

宇宙学与河外天体物理 · 物理学 2015-05-13 H. -R. Kloeckner , A. Martinez-Sansigre , S. Rawlings , M. A. Garrett

We present continuum observations of a small sample of high-redshift, radio-loud AGN (radio galaxies and quasars) aimed at the detection of thermal emission from dust. Seven AGN were observed with IRAM and SEST at 1.25mm; two of them, the…

天体物理学 · 物理学 2007-05-23 Andrea Cimatti , Wolfram Freudling , Huub Roettgering , Rob Ivison , Paola Mazzei

Models and observations suggest that luminous quasar activity is triggered by mergers, so it should preferentially occur in the most massive primordial dark matter haloes, where the frequency of mergers is expected to be the highest. Since…

星系天体物理 · 物理学 2018-04-04 C. Vignali , E. Piconcelli , M. Perna , J. Hennawi , R. Gilli , A. Comastri , G. Zamorani , M. Dotti , S. Mathur

HE0450-2958, an interacting quasar-starburst galaxy pair at $z$ = 0.285, is one of the best known examples of strong star formation activity in the presence of a quasar-driven jet. We present new multi-band JVLA-imaging covering 1 to 6 GHz…

星系天体物理 · 物理学 2017-03-20 Daniel Cs. Molnar , Mark T. Sargent , David Elbaz , Padelis P. Papadopoulos , Joseph Silk

Signatures of the re-occurrence of activity in radio-loud AGNs, indicated either by the so-called double-double or X-shaped structures, have been observed in a number of radio sources. All such objects known to date have linear sizes of the…

天体物理学 · 物理学 2009-11-13 A. Marecki , P. Thomasson , K. -H. Mack , M. Kunert-Bajraszewska

Giant double-lobed radio source 4C34.47 displays a straight one-sided jet, measuring a record length of 380kpc, in its double-lobed radio structure. Assuming an intrinsically symmetric two-sided jet structure the radio source jet axis must…

星系天体物理 · 物理学 2015-05-19 S. Hocuk , P. D. Barthel

We report on two surveys of radio-weak AGN to look for radio variability. We find significant variability with an RMS of 10-20% on a timescale of months in radio-quiet and radio-intermediate quasars. This exceeds the variability of radio…

天体物理学 · 物理学 2007-05-23 Heino Falcke , Joseph Lehar , Richard Barvainis , Neil M. Nagar , Andrew S. Wilson

We present optical (~3200A to ~9000A) off-nuclear spectra of 26 powerful active galaxies in the redshift range 0.1 < z < 0.3, obtained with the Mayall and William Herschel 4-meter class telescopes. The sample consists of radio-quiet…

天体物理学 · 物理学 2009-10-31 David H. Hughes , Marek J. Kukula , James S. Dunlop , Todd Boroson

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 present deep Giant Metrewave Radio Telescope (GMRT) radio observations at 240, 330 and 610 MHz of the complex radio source at the center of the NGC1407 galaxy group. Previous GMRT observations at 240 MHz revealed faint, diffuse emission…

We report here on the discovery of a red quasar, J004929.4+351025.7 at a redshift of z = 2.48, situated within a large Lya emission-line halo. The radio spectral energy distribution implies that the radio jets were triggered < 10^4 years…

Active galactic nuclei and quasars are thought to be scaled up versions of Galactic black hole binaries, powered by accretion onto supermassive black holes with masses of 10^6-10^9 M_Sun, as opposed to the ~10 M_Sun in binaries. One example…

天体物理学 · 物理学 2008-07-14 Marek Gierlinski , Matthew Middleton , Martin Ward , Chris Done

Many low-luminosity active galactic nuclei (AGNs) contain a compact radio core which can be observed with high angular resolution using very long baseline interferometry (VLBI). Combining arcsec-scale structural information with…

星系天体物理 · 物理学 2020-04-06 Máté Krezinger , Sándor Frey , Zsolt Paragi , Roger Deane

IRAS 09104+4109 is a rare example of a dust enshrouded type 2 QSO in the centre of a cool-core galaxy cluster. Previous observations of this z=0.44 system showed that as well as powering the hyper-luminous infrared emission of the…

Blazars are active galactic nuclei (AGN) whose relativistic jets point nearly to the line of sight. Their compact radio structure can be imaged with very long baseline interferometry (VLBI) on parsec scales. Blazars at extremely high…

星系天体物理 · 物理学 2017-02-12 H. -M. Cao , S. Frey , K. É. Gabányi , Z. Paragi , J. Yang , D. Cseh , X. -Y. Hong , T. An