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相关论文: Evidence for Wide-Spread AGN Driven Outflows in th…

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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…

星系天体物理 · 物理学 2017-03-15 Hyun-Jin Bae , Jong-Hak Woo , Marios Karouzos , Elena Gallo , Helene Flohic , Yue Shen , Suk-Jin Yoon

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…

星系天体物理 · 物理学 2015-06-18 Jared M. Gabor , Frédéric Bournaud

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…

高能天体物理现象 · 物理学 2018-09-21 E. de Gouveia Dal Pino , W. Clavijo-Bohórquez , C. Melioli

Ionised gas outflows driven by active galactic nuclei (AGN) are ubiquitous in high luminosity AGN with outflow speeds apparently correlated with the total bolometric luminosity of the AGN. This empirical relation and theoretical work…

Using a sample of 2922 z<0.2, spectroscopically-identified Active Galactic Nuclei (AGN) we explore the relationship between radio size and the prevalence of extreme ionised outflows, as traced using broad [O III] emission-line profiles in…

星系天体物理 · 物理学 2019-11-06 S. J. Molyneux , C. M. Harrison , M. E. Jarvis

Outflows have been shown to be prevalent in galaxies hosting luminous active galactic nuclei (AGNs) and present a physically plausible way to couple the AGN energy output with the interstellar medium of their hosts. Despite their…

星系天体物理 · 物理学 2016-12-21 Marios Karouzos , Jong-Hak Woo , Hyun-Jin Bae

We show the effects of AGN-driven outflows on the ejection of heavy elements using our cosmological simulations, where super-massive black holes originate from the first stars. In the most massive galaxy, we have identified two strong…

星系天体物理 · 物理学 2015-08-06 Philip Taylor , Chiaki Kobayashi

We study molecular outflows in a sample of 45 local galaxies, both star forming and AGN, primarily by using CO data from the ALMA archive and from the literature. For a subsample we also compare the molecular outflow with the ionized and…

星系天体物理 · 物理学 2019-02-27 A. Fluetsch , R. Maiolino , S. Carniani , A. Marconi , C. Cicone , M. A. Bourne , T. Costa , A. C. Fabian , W. Ishibashi , G. Venturi

We present an optical spectroscopic study of a 90% complete sample of 17 nearby ULIRGs with optical Seyfert nuclei, with the aim of investigating the nature of the nuclear warm gas outflows. A high proportion (94%) of our sample show…

宇宙学与河外天体物理 · 物理学 2015-06-15 J. Rodriguez Zaurin , C. N. Tadhunter , M. Rose , J. Holt

Active Galactic Nuclei (AGNs) exhibit excess mid-infrared H$_2$ emission compared to star-forming galaxies, likely driven by outflows and shocks inferred from integrated spectra. We present optical IFU observations of the central 2\,kpc of…

Large scale, weakly collimated outflows are very common in galaxies with large infrared luminosities. In complex systems in particular, where intense star formation (SF) coexists with an active galactic nucleus (AGN), it is not clear yet…

星系天体物理 · 物理学 2015-10-21 Claudio Melioli , Elisabete M. de Gouveia Dal Pino

We use the sample of emission-line nuclei derived from a recently completed optical spectroscopic survey of nearby galaxies to quantify the incidence of local (z = 0) nuclear activity. Consistent with previous studies, we find detectable…

天体物理学 · 物理学 2009-10-30 Luis C. Ho , Alexei V. Filippenko , Wallace L. W. Sargent

We present statistics of $z\sim 6-9$ galaxy outflows indicated by spatially-extended gas emission and broad lines. With a total of 61 spectroscopically confirmed galaxies at $z\sim 6-9$ in the JWST CEERS, GLASS, and ERO data, we find four…

星系天体物理 · 物理学 2024-05-09 Yechi Zhang , Masami Ouchi , Kimihiko Nakajima , Yuichi Harikane , Yuki Isobe , Yi Xu , Yoshiaki Ono , Hiroya Umeda

We present a sample of 398 galaxies with ionized gas outflow signatures in their spectra from the Galaxy and Mass Assembly (GAMA) Survey Data Release 4, including 45 low-mass galaxies with stellar masses $M_*<10^{10}$ $M_\odot$. We assemble…

星系天体物理 · 物理学 2024-12-03 Sheyda Salehirad , Amy E. Reines , Mallory Molina

Several models have predicted that stars could form inside galactic outflows and that this would be a new major mode of galaxy evolution. Observations of galactic outflows have revealed that they host large amounts of dense and clumpy…

星系天体物理 · 物理学 2019-03-06 R. Gallagher , R. Maiolino , F. Belfiore , N. Drory , R. Riffel , R. A. Riffel

We present subarcsecond resolution mid-infrared (MIR) images obtained with 8-10 m-class ground-based telescopes of a complete volume-limited (DL<40 Mpc) sample of 24 Seyfert galaxies selected from the Swift/BAT nine month catalog. We use…

Some cosmological hydrodynamical simulations predict that outflows driven by active galactic nuclei (AGN) play a key role in powering the Ly$\alpha$ nebulae observed around high-redshift quasars. In such simulations, AGN feedback seeded as…

We present spatially resolved rest-optical spectroscopy of 38 star-forming galaxies at 0.5 < z < 1.7 from the JWST/NIRSpec MSA-3D survey, which uses slit-stepping to build IFU-like datacubes at 0.1'' resolution. We map emission-line…

Active galactic nuclei (AGN) feedback operated by the expansion of radio jets can play a crucial role in driving gaseous outflows on galaxy scales. Galaxies hosting young radio AGN, whose jets are in the first phases of expansion through…

星系天体物理 · 物理学 2021-01-04 F. Santoro , C. Tadhunter , D. Baron , R. Morganti , J. Holt