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Related papers: Neutral Gas Outflows and Inflows in Infrared-Faint…

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The study of winds in active galactic nuclei (AGN) is of utmost importance as they may provide the long sought-after link between the central black hole and the host galaxy, establishing the AGN feedback. Recently, Laha et al. (2014)…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Francesco Tombesi , Massimo Cappi

Relativistically blueshifted absorption features of highly ionised ions, the so-called ultra-fast outflows (UFOs), have been detected in the X-ray spectra of a number of accreting supermassive black holes. If these features truly originate…

High Energy Astrophysical Phenomena · Physics 2020-06-03 P. Kosec , A. Zoghbi , D. J. Walton , C. Pinto , A. C. Fabian , M. L. Parker , C. S. Reynolds

We present the first systematic study of the molecular gas and star formation efficiency in a sample of ten narrow-line Seyfert 1 galaxies selected to have X-ray Ultra Fast Outflows and, therefore, to potentially show AGN feedback effects.…

To investigate AGN outflows as a tracer of AGN feedback on star-formation, we perform integral-field spectroscopy of 20 type 2 AGNs at z<0.1, which are luminous AGNs with the [O III] luminosity >10$^{41.5}$ erg/s, and exhibit strong outflow…

Astrophysics of Galaxies · Physics 2017-03-15 Hyun-Jin Bae , Jong-Hak Woo , Marios Karouzos , Elena Gallo , Helene Flohic , Yue Shen , Suk-Jin Yoon

Large-scale, broad outflows are common in active galaxies. In systems where star formation coexists with an AGN, it is unclear yet the role that both play on driving the outflows. In this work we present three-dimensional radiative-cooling…

High Energy Astrophysical Phenomena · Physics 2018-09-21 E. de Gouveia Dal Pino , W. Clavijo-Bohórquez , C. Melioli

The existence of ionized X-ray absorbing layers of gas along the line of sight to the nuclei of Seyfert galaxies is a well established observational fact. This material is systematically outflowing and shows a large range in parameters.…

High Energy Astrophysical Phenomena · Physics 2015-06-12 F. Tombesi , M. Cappi , J. N. Reeves , R. S. Nemmen , V. Braito , M. Gaspari , C. S. Reynolds

We study outflows driven by Active Galactic Nuclei (AGNs) using high- resolution simulations of idealized z=2 isolated disk galaxies. Episodic accretion events lead to outflows with velocities >1000 km/s and mass outflow rates up to the…

Astrophysics of Galaxies · Physics 2015-06-18 Jared M. Gabor , Frédéric Bournaud

Feedback from active galactic nuclei (AGN) is widely considered to be the main driver in regulating the growth of massive galaxies through heating or driving gas out of the galaxy, preventing further increase in stellar mass. Observational…

Astrophysics of Galaxies · Physics 2016-08-03 Dominika Wylezalek , Nadia L. Zakamska

In this paper, we present moderately-high resolution (~65 km/s) spectroscopy, acquired with ESI on Keck II, of 11 ultraluminous infrared galaxies at z < 0.3 from the IRAS 1 Jy sample. The targets were chosen as good candidates to host…

Astrophysics · Physics 2009-11-07 David S. Rupke , Sylvain Veilleux , D. B. Sanders

We use optical spectra from the inner 2$\times$3kpc$^2$ of the Seyfert 2 galaxy NGC1667, obtained with the GMOS integral field spectrograph on the Gemini South telescope at a spatial resolution of $\approx$ 240pc, to assess the feeding and…

Astrophysics of Galaxies · Physics 2017-01-18 Allan Schnorr-Müller , Thaisa Storchi-Bergmann , Fabricio Ferrari , Neil M. Nagar

Far-Infrared (FIR) photometry from the the Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory is presented for 313 nearby, hard X-ray selected galaxies from the 58-month Swift Burst Alert Telescope (BAT)…

Astrophysics of Galaxies · Physics 2015-06-22 M. Meléndez , R. F. Mushotzky , T. T. Shimizu , A. J. Barger , L. L. Cowie

We report on a S/N-limited search for low-ionization gas outflows in the spectra of the 0.11 < z < 0.54 objects in the EGS portion of the DEEP2 survey. Doppler shifts from the host galaxy redshifts are systematically searched for in the Na…

Astrophysics · Physics 2015-03-13 Taro Sato , Crystal L. Martin , Kai G. Noeske , David C. Koo , Jennifer M. Lotz

We present mid-infrared data of a sample of 57 AGNs obtained with the instrument ISOCAM on board the satellite ISO. The images were obtained through the LW2 (6.75 microns) and LW7 (9.62 microns) filters. This is a new analysis of Clavel et…

The properties of large-scale galactic outflows, such as their kinetic energy and momentum rates, correlate with the luminosity of the active galactic nucleus (AGN). This is well explained by the wind-driven outflow model, where a fraction…

Astrophysics of Galaxies · Physics 2020-09-30 Kastytis Zubovas , Emanuele Nardini

We report on the determination of electron densities, and their impact on the outflow masses and rates, measured in the central few hundred parsecs of 11 local luminous active galaxies. We show that the peak of the integrated line emission…

Infrared photometry and later infrared spectroscopy provided powerful diagnostics to distinguish between the main emission mechanisms in galaxies: AGN and Starburst. After the pioneering work on infrared photometry with IRAS in the far-IR…

Astrophysics of Galaxies · Physics 2009-01-23 Luigi Spinoglio , Silvia Tommasin , Matthew A. Malkan

Dusty, neutral outflows and inflows are a common feature of nearby star-forming galaxies. We characterize these flows in eight galaxies -- mostly AGN -- selected for their widespread NaI D signatures from the Siding Spring Southern Seyfert…

Astrophysics of Galaxies · Physics 2021-03-24 David S. N. Rupke , Adam D. Thomas , Michael A. Dopita

New far-infrared photometry with ISOPHOT, onboard the Infrared Space Observatory, is presented for 58 galaxies with homogeneous published data for another 32 galaxies all belonging to the 12 micron galaxy sample. In total 29 Seyfert 1's, 35…

Astrophysics · Physics 2009-11-07 Luigi Spinoglio , Paola Andreani , Matthew A. Malkan

We collate the results of recent high resolution X-ray spectroscopic observations of 23 AGN, and use the resulting information to try to provide answers to some of the main open questions about warm absorbers: where do they originate, what…

Astrophysics · Physics 2009-11-10 A. J. Blustin , M. J. Page , S. V. Fuerst , G. Branduardi-Raymont , C. E. Ashton