FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3103859359> ?p ?o ?g. }

• W3103859359 endingPage "28" @default.
• W3103859359 startingPage "28" @default.
• W3103859359 abstract "We use deep adaptive optics assisted integral field spectroscopy from SINFONI on the VLT to study the spatially resolved properties of ionized gas outflows driven by active galactic nuclei (AGNs) in three galaxies at z ∼ 2.2—K20-ID5, COS4-11337, and J0901 + 1814. These systems probe AGN feedback from nuclear to circumgalactic scales and provide unique insights into the different mechanisms by which AGN-driven outflows interact with their host galaxies. K20-ID5 and COS4-11337 are compact star-forming galaxies with powerful ∼1500 km s−1 AGN-driven outflows that dominate their nuclear Hα emission. The outflows do not appear to have any impact on the instantaneous star formation activity of the host galaxies, but they carry a significant amount of kinetic energy that could heat the halo gas and potentially lead to a reduction in the rate of cold gas accretion onto the galaxies. The outflow from COS4-11337 is propagating directly toward its companion galaxy COS4-11363, at a projected separation of 5.4 kpc. COS4-11363 shows signs of shock excitation and recent truncation of star formation activity, which could plausibly have been induced by the outflow from COS4-11337. J0901 + 1814 is gravitationally lensed, giving us a unique view of a compact (R = 470 ± 70 pc), relatively low-velocity (∼650 km s−1) AGN-driven outflow. J0901 + 1814 has a similar AGN luminosity to COS4-11337, suggesting that the difference in outflow properties is not related to the current AGN luminosity and may instead reflect a difference in the evolutionary stage of the outflow and/or the coupling efficiency between the AGN ionizing radiation field and the gas in the nuclear regions." @default.
• W3103859359 created "2020-11-23" @default.
• W3103859359 creator A5004404122 @default.
• W3103859359 creator A5010471147 @default.
• W3103859359 creator A5022575311 @default.
• W3103859359 creator A5023265038 @default.
• W3103859359 creator A5032049136 @default.
• W3103859359 creator A5036816181 @default.
• W3103859359 creator A5043955323 @default.
• W3103859359 creator A5047003495 @default.
• W3103859359 creator A5052954301 @default.
• W3103859359 creator A5060901790 @default.
• W3103859359 creator A5063959023 @default.
• W3103859359 creator A5067573740 @default.
• W3103859359 creator A5069212337 @default.
• W3103859359 creator A5084296896 @default.
• W3103859359 creator A5086194401 @default.
• W3103859359 creator A5087379508 @default.
• W3103859359 creator A5088790406 @default.
• W3103859359 creator A5091386388 @default.
• W3103859359 date "2020-05-01" @default.
• W3103859359 modified "2023-10-01" @default.
• W3103859359 title "From Nuclear to Circumgalactic: Zooming in on AGN-driven Outflows at <i>z</i> ∼ 2.2 with SINFONI" @default.
• W3103859359 cites W1683186775 @default.
• W3103859359 cites W1911322997 @default.
• W3103859359 cites W1920334662 @default.
• W3103859359 cites W1921256341 @default.
• W3103859359 cites W1977361870 @default.
• W3103859359 cites W1981936828 @default.
• W3103859359 cites W1988295528 @default.
• W3103859359 cites W1990491187 @default.
• W3103859359 cites W1992371393 @default.
• W3103859359 cites W1994671833 @default.
• W3103859359 cites W1998014385 @default.
• W3103859359 cites W2002044265 @default.
• W3103859359 cites W2004977915 @default.
• W3103859359 cites W2005798315 @default.
• W3103859359 cites W2011301426 @default.
• W3103859359 cites W2011654732 @default.
• W3103859359 cites W2014181843 @default.
• W3103859359 cites W2014220424 @default.
• W3103859359 cites W2014726262 @default.
• W3103859359 cites W2016904340 @default.
• W3103859359 cites W2019562528 @default.
• W3103859359 cites W2024319723 @default.
• W3103859359 cites W2024833278 @default.
• W3103859359 cites W2025335970 @default.
• W3103859359 cites W2027713091 @default.
• W3103859359 cites W2031617522 @default.
• W3103859359 cites W2033803356 @default.
• W3103859359 cites W2034288205 @default.
• W3103859359 cites W2034343521 @default.
• W3103859359 cites W2039304323 @default.
• W3103859359 cites W2040503929 @default.
• W3103859359 cites W2048414711 @default.
• W3103859359 cites W2049052485 @default.
• W3103859359 cites W2053222813 @default.
• W3103859359 cites W2054103046 @default.
• W3103859359 cites W2054487943 @default.
• W3103859359 cites W2059634633 @default.
• W3103859359 cites W2066396108 @default.
• W3103859359 cites W2069396164 @default.
• W3103859359 cites W2070431442 @default.
• W3103859359 cites W2071737440 @default.
• W3103859359 cites W2075056822 @default.
• W3103859359 cites W2079227246 @default.
• W3103859359 cites W2084264738 @default.
• W3103859359 cites W2085005802 @default.
• W3103859359 cites W2086949239 @default.
• W3103859359 cites W2087525524 @default.
• W3103859359 cites W2090459210 @default.
• W3103859359 cites W2091163781 @default.
• W3103859359 cites W2092504858 @default.
• W3103859359 cites W2101300883 @default.
• W3103859359 cites W2106221033 @default.
• W3103859359 cites W2107308864 @default.
• W3103859359 cites W2114561384 @default.
• W3103859359 cites W2117943668 @default.
• W3103859359 cites W2119131940 @default.
• W3103859359 cites W2120523711 @default.
• W3103859359 cites W2124821818 @default.
• W3103859359 cites W2130290556 @default.
• W3103859359 cites W2135625048 @default.
• W3103859359 cites W2137397364 @default.
• W3103859359 cites W2151062050 @default.
• W3103859359 cites W2159473840 @default.
• W3103859359 cites W2162475780 @default.
• W3103859359 cites W2163032978 @default.
• W3103859359 cites W2167012389 @default.
• W3103859359 cites W2167635287 @default.
• W3103859359 cites W2170769203 @default.
• W3103859359 cites W2200610228 @default.
• W3103859359 cites W2291265024 @default.
• W3103859359 cites W2401435175 @default.
• W3103859359 cites W2468373122 @default.
• W3103859359 cites W2503926030 @default.
• W3103859359 cites W2508402256 @default.
• W3103859359 cites W2510079733 @default.

• next