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Nest200047 is a clear example of multiple radio bubbles from an Active Galactic Nucleus (AGN) in a galaxy group, featuring non-thermal filaments likely shaped by buoyancy, gas motions, and stabilized by magnetic fields. This study presents…

We report the discovery of a luminous ultra-soft X-ray excess in a radio-loud narrow-line Seyfert1 galaxy, RXJ1633+4718, from archival ROSAT observations. The thermal temperature of this emission, when fitted with a blackbody, is as low as…

高能天体物理现象 · 物理学 2015-05-19 Weimin Yuan , Bifang Liu , Hongyan Zhou , Tinggui Wang

M87 hosts a 3-6 billion solar mass black hole with a remarkable relativistic jet that has been regularly monitored in radio to TeV bands. However, hard X-ray emission \gtrsim 10keV, which would be expected to primarily come from the jet or…

高能天体物理现象 · 物理学 2017-11-07 Ka-Wah Wong , Rodrigo S. Nemmen , Jimmy A. Irwin , Dacheng Lin

We investigate the dichotomy between jetted and non-jetted Active Galactic Nuclei (AGNs), focusing on the fundamental differences of these two classes in the accretion physics onto the central supermassive black hole (SMBH). Our aim is to…

高能天体物理现象 · 物理学 2019-07-18 Samuele Ronchini , Francesco Tombesi , Fausto Vagnetti , Francesca Panessa , Gabriele Bruni

Type 2 active galactic nuclei (AGN) show signatures of accretion onto a supermassive black hole through strong, high-ionization, narrow emission lines extended on scales of 100s to 1000s of parsecs, but they lack the broad emission lines…

高能天体物理现象 · 物理学 2022-09-21 M. Lynne Saade , Murray Brightman , Daniel Stern , Matthew A. Malkan , Javier A. Garcia

Supermassive black hole feedback is the currently favoured mechanism to regulate the star formation rate of galaxies and prevent the formation of ultra-massive galaxies ($M_\star>10^{12}M_\odot$). However, the mechanism through which the…

As a newly discovered class of radio-loud active galactic nuclei (AGNs), the \gamma-ray detected narrow-line Seyfert 1 galaxies (NLS1s) launch powerful jets which are generally found only in blazars and radio galaxies. However, their black…

高能天体物理现象 · 物理学 2019-03-15 Hai-Wu Pan , Weimin Yuan , Su Yao , S. Komossa , Chichuan Jin

We present a sample of accreting supermassive black holes (SMBHs) in dwarf galaxies at $z<1$. We identify dwarf galaxies in the NEWFIRM Medium Band Survey with stellar masses $M_{\star}<3\times 10^{9} M_{\odot}$ that have spectroscopic…

The cores of active galactic nuclei (AGN) harbor some of the most extreme conditions of matter and energy in the Universe. One of the major goals of high-energy astrophysics is to probe these extreme environments in the vicinity of…

天体物理学 · 物理学 2009-10-31 K. A. Weaver

We investigate the role of host galaxy classification and black hole mass in a heterogeneous sample of 276 mostly nearby (z<0.1) X-ray and IR selected AGN. Around 90% of Seyfert 1 AGN in bulge-dominated host galaxies (without disk…

宇宙学与河外天体物理 · 物理学 2015-05-19 Barry McKernan , K. E. Saavik Ford , Chris Reynolds

As matter accretes onto the central supermassive black holes in active galactic nuclei (AGN), X-rays are emitted. We present a population synthesis model that accounts for the summed X-ray emission from growing black holes; modulo the…

We present a clustering analysis of X-ray selected AGN by compiling X-ray samples from the literature and re-estimating the dark matter (DM) halo masses of AGN in a uniform manner. We find that moderate luminosity AGN (Lx(2-10…

宇宙学与河外天体物理 · 物理学 2015-06-15 N. Fanidakis , A. Georgakakis , G. Mountrichas , M. Krumpe , C. M. Baugh , C. G. Lacey , C. S. Frenk , T. Miyaji , A. J. Benson

Recent studies of active galactic nuclei (AGN) found a statistical inverse linear scaling between the X-ray normalized excess variance $\sigma_{\rm rms}^2$ (variability amplitude) and the black hole mass spanning over $M_{\rm BH}=10^6-…

高能天体物理现象 · 物理学 2015-06-26 Hai-Wu Pan , Weimin Yuan , Xin-Lin Zhou , Xiao-Bo Dong , Bifang Liu

Active galactic nuclei (AGN) play a crucial role in galaxy evolution by influencing the observational properties of their host galaxies. We investigate the host galaxy properties of X-ray selected AGNs, focusing on differences between…

星系天体物理 · 物理学 2025-08-28 Carlos G. Bornancini , Gabriel A. Oio , Georgina Coldwell

We analyse the spectra of the archival XMM-Newton data of the Seyfert 1 AGN Zw 229.015 in the energy range $0.3 - 10.0$ keV. When fitted with a simple power-law, the spectrum shows signatures of weak soft excess below 1.0 keV. We find that…

星系天体物理 · 物理学 2016-12-21 Oluwashina Adegoke , Suvendu Rakshit , Banibrata Mukhopadhyay

By analyzing Chandra X-ray data of a sample of 21 galaxy groups and 19 galaxy clusters, we find that in 31 sample systems there exists a significant central ($R^{<}_{\sim} 10h_{71}^{-1}$ kpc) gas entropy excess ($\Delta K_{0}$), which…

宇宙学与河外天体物理 · 物理学 2015-05-19 Yu Wang , Haiguang Xu , Junhua Gu , Liyi Gu , Jingying Wang , Zhongli Zhang

Recent X-ray observations of hot gas in the galaxy cluster MS 0735.6+7421 reveal huge radio-bright, quasi-bipolar X-ray cavities having a total energy ~10^{62} ergs, the most energetic AGN outburst currently known. We investigate the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Fulai Guo , William G. Mathews

NGC 4993, as a host galaxy of the electromagnetic counterpart of the first gravitational-wave detection of a binary neutron-star merger, was observed by many powerful telescopes from radio to $\gamma$-ray waveband. The weak nuclear…

高能天体物理现象 · 物理学 2018-03-21 Qingwen Wu , Jianchao Feng , Xuliang Fan

Accretion states, which are universally observed in stellar-mass black holes in X-ray binaries, are also anticipated in active galactic nuclei (AGN). This is the case at low luminosities, when the jet-corona coupling dominates the energy…

高能天体物理现象 · 物理学 2021-04-28 Juan A. Fernández-Ontiveros , Teo Muñoz-Darias

We present an ongoing study of 18 nearby galaxy groups, chosen for the availability of Chandra and/or XMM-Newton data and evidence for AGN/hot intragroup gas interaction. We have obtained 235 and 610 MHz observations at the GMRT for all the…

宇宙学与河外天体物理 · 物理学 2015-05-14 S. Giacintucci , J. M. Vrtilek , E. O'Sullivan , S. Raychaudhury , L. P. David , T. Venturi , R. Athreya , M. Gitti
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