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相关论文: The parsec-scale HI outflows in powerful radio gal…

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The feedback from an active galactic nucleus (AGN) is frequently invoked as a mechanism through which gas can be heated or removed from a galaxy. However, gas fraction measurements in AGN hosts have yielded mixed support for this scenario.…

星系天体物理 · 物理学 2018-12-12 Sara L. Ellison , Toby Brown , Barbara Catinella , Luca Cortese

Massive gas outflows are considered a key component in the process of galaxy formation and evolution. Because of this, they are the topic of many studies aimed at learning more about their occurrence, location and physical conditions as…

星系天体物理 · 物理学 2015-06-23 Raffaella Morganti

We report the results of Giant Metrewave Radio Telescope (GMRT) observations of H{\sc i} absorption towards the FRII radio galaxy 3C321 (J1531+2404), which is associated with an active galaxy interacting with a companion. The absorption…

星系天体物理 · 物理学 2012-08-16 Yogesh Chandola , S. K. Sirothia , D. J. Saikia , Neeraj Gupta

X-ray absorption line spectroscopy has recently shown evidence for previously unknown Ultra-fast Outflows (UFOs) in radio-quiet AGNs. In the previous paper of this series we defined UFOs as those absorbers with an outflow velocity higher…

高能天体物理现象 · 物理学 2015-05-30 F. Tombesi , M. Cappi , J. N. Reeves , G. G. C. Palumbo , V. Braito , M. Dadina

Flares in radio-loud AGN are thought to be associated with the injection of fresh plasma into the compact jet base. Such flares are usually strongest and appear earlier at shorter radio wavelengths. Hence, VLBI at mm-wavelengths is best…

高能天体物理现象 · 物理学 2021-01-04 R. Schulz , M. Kadler , E. Ros , M. Perucho , T. P. Krichbaum , I. Agudo , T. Beuchert , M. Lindqvist , K. Mannheim , J. Wilms , J. A. Zensus

We have analyzed new, archival and published high resolution radio and X-ray observations of a sample of composite LINER/HII galaxies known to exhibit AGN-like properties. Five of the 16 AGN candidates have milliarcsecond-scale detections…

天体物理学 · 物理学 2009-11-10 M. E. Filho , F. Fraternali , S. Markoff , N. M. Nagar , P. D. Barthel , L. C. Ho , F. Yuan

Active galactic nucleus (AGN) feedback is postulated as a key mechanism for regulating star formation within galaxies. Studying the physical properties of the outflowing gas from AGN is thus crucial for understanding the co-evolution of…

One of the main debated astrophysical problems is the role of the AGN feedback in galaxy formation. It is known that massive black holes have a profound effect on the formation and evolution of galaxies, but how black holes and galaxies…

高能天体物理现象 · 物理学 2015-06-03 E. Torresi , P. Grandi , E. Costantini , G. G. C. Palumbo

We examine how HI and metal absorption lines within low-redshift galaxy halos trace the dynamical state of circumgalactic gas, using cosmological hydrodynamic simulations that include a well-vetted heuristic model for galactic outflows. We…

宇宙学与河外天体物理 · 物理学 2015-06-17 Amanda Brady Ford , Romeel Davé , Benjamin D. Oppenheimer , Neal Katz , Juna A. Kollmeier , Robert Thompson , David H. Weinberg

We investigate the global neutral hydrogen (HI) content of isolated galaxies selected from the SDSS spectroscopic survey with optical evidence of Active Galactic Nuclei (AGN). Our sample includes galaxies with unresolved HI observations…

星系天体物理 · 物理学 2018-07-18 Jeremy D. Bradford , Marla C. Geha , Jenny E. Greene , Amy E. Reines , Claire M. Dickey

We present global VLBI observations of the ~8100 km s$^{-1}$ HI absorption feature detected toward the strong radio nucleus 3C 84 of NGC 1275 in the Perseus cluster (${V_{\rm sys}\sim}$5200 km s$^{-1}$). The observations were obtained using…

天体物理学 · 物理学 2009-11-07 E. Momjian , J. D. Romney , T. H. Troland

This is the first paper of a series exploring the multi-frequency properties of a sample of eleven nearby low excitation radio galaxies (LERGs) in the southern sky. We are conducting an extensive study of different galaxy components (stars,…

The study of neutral hydrogen emission and absorption in radio galaxies is giving new and important insights on a variety of phenomena observed in these objects. Such observations are helping to understand the origin of the host galaxy, the…

天体物理学 · 物理学 2009-11-11 Raffaella Morganti

A pilot study with the powerful new backend of the Westerbork Synthesis Radio Telescope (WSRT) of two galaxy clusters at z=0.2 has revealed neutral hydrogen emission from 39 galaxies. The volume probed for each cluster is 1.7x10^4 Mpc^3,…

Nearby interstellar clouds with high (|v| >/= 10 km/s) random velocities although easily detected in NaI and CaII lines have hitherto not been detected (in emission or absorption) in the HI 21cm line. We describe here deep Giant Metrewave…

天体物理学 · 物理学 2009-11-06 Rekhesh Mohan , K. S. Dwarakanath , G. Srinivasan , Jayaram N. Chengalur

We present new, high angular resolution (~0.22") MERLIN observations of neutral hydrogen (HI) absorption and 21-cm radio continuum emission across the central ~900 parsecs of the ultraluminous infrared galaxy, Arp220. Spatially resolved HI…

天体物理学 · 物理学 2009-11-06 C. G. Mundell , P Ferruit , A Pedlar

Observations of the neutral atomic hydrogen (HI) in the nuclear starburst galaxy NGC 4945 with MeerKAT are presented. We find a large amount of halo gas, previously missed by HI observations, accounting for 6.8% of the total HI mass. This…

The driving force behind outflows, often invoked to understand the correlation between the supermassive black holes powering active galactic nuclei (AGN) and their host galaxy properties, remains uncertain. We provide new insights into the…

星系天体物理 · 物理学 2025-03-11 Payel Nandi , C. S. Stalin , D. J. Saikia

Aims. We investigate the different manifestations of AGN feedback in the evolved, powerful radio source 3C293 and their impact on the molecular gas of its host galaxy, which harbors young star-forming regions and fast outflows of HI and…

星系天体物理 · 物理学 2014-05-08 A. Labiano , S. Garcia-Burillo , F. Combes , A. Usero , R. Soria-Ruiz , J. Piqueras Lopez , A. Fuente. , L. Hunt , R Neri

We present MeerKAT observations searching for HI absorption in a sample of 17 powerful ($L_{\rm 1.4GHz}> 10^{27}$ W Hz$^{-1}$) radio sources at intermediate redshifts ($0.25<z<0.7$). The sample is well characterised at radio and optical…

星系天体物理 · 物理学 2026-02-11 Raffaella Morganti , Tom Oosterloo , Clive Tadhunter , Suma Murthy