Matches in SemOpenAlex for { <https://semopenalex.org/work/W2931769884> ?p ?o ?g. }
- W2931769884 endingPage "29" @default.
- W2931769884 startingPage "29" @default.
- W2931769884 abstract "We present ALMA rest-frame 230 GHz continuum and CO(2-1) line observations of the nearby Compton-thick Seyfert galaxy ESO428-G14, with angular resolution 0.7 arcsec (78 pc). We detect CO(2-1) emission from spiral arms and a circum-nuclear ring with 200 pc radius, and from a transverse gas lane with size of $sim100$ pc, which crosses the nucleus and connects the two portions the circumnuclear ring. The molecular gas in the host galaxy is distributed in a rotating disk with intrinsic circular velocity $v_{rot}=135$ km/s, inclination $i=57$ deg, and dynamical mass $M_{dyn }=5times 10^9~rm M_{odot}$ within a radius of $sim 1$ kpc. In the inner 100 pc region CO is distributed in a equatorial bar, whose kinematics is highly perturbed and consistent with an inflow of gas towards the AGN. This inner CO bar overlaps with the most obscured, Compton-thick region seen in X-rays. We derive a column density of $rm N(H_2) approx 2times10^{23}~ cm^{-2}$ in this region, suggesting that molecular gas may contribute significantly to the AGN obscuration. We detect a molecular outflow with a total outflow rate $rm dot M_{of}approx 0.8~M_{odot}/yr$, distributed along a bi-conical structure with size of $700$ pc on both sides of the AGN. The bi-conical outflow is also detected in the $rm H_2$ emission line at 2.12 $mu$m, which traces a warmer nuclear outflow located within 170 pc from the AGN. This suggests that the outflow cools with increasing distance from the AGN. We find that the hard X-ray emitting nuclear region mapped with Chandra is CO-deprived, but filled with warm molecular gas traced by $rm H_2$ - thus confirming that the hard (3-6 keV) continuum and Fe K$alpha$ emission are due to scattering from dense neutral clouds in the ISM." @default.
- W2931769884 created "2019-04-11" @default.
- W2931769884 creator A5002705377 @default.
- W2931769884 creator A5007779776 @default.
- W2931769884 creator A5016187719 @default.
- W2931769884 creator A5039128270 @default.
- W2931769884 creator A5051825718 @default.
- W2931769884 creator A5080029324 @default.
- W2931769884 date "2020-02-10" @default.
- W2931769884 modified "2023-10-05" @default.
- W2931769884 title "Multiphase Gas Flows in the Nearby Seyfert Galaxy ESO428–G014. Paper I" @default.
- W2931769884 cites W1925665838 @default.
- W2931769884 cites W1926815209 @default.
- W2931769884 cites W1990401433 @default.
- W2931769884 cites W2016158860 @default.
- W2931769884 cites W2026082409 @default.
- W2931769884 cites W2083471080 @default.
- W2931769884 cites W2087932781 @default.
- W2931769884 cites W2096336682 @default.
- W2931769884 cites W2128026040 @default.
- W2931769884 cites W2145089139 @default.
- W2931769884 cites W2147040512 @default.
- W2931769884 cites W2148005077 @default.
- W2931769884 cites W2155421027 @default.
- W2931769884 cites W2331530014 @default.
- W2931769884 cites W2589201834 @default.
- W2931769884 cites W2617266012 @default.
- W2931769884 cites W2806944713 @default.
- W2931769884 cites W2888625348 @default.
- W2931769884 cites W2888630964 @default.
- W2931769884 cites W2941054934 @default.
- W2931769884 cites W2962267076 @default.
- W2931769884 cites W3098951039 @default.
- W2931769884 cites W3099533589 @default.
- W2931769884 cites W3100066963 @default.
- W2931769884 cites W3100264713 @default.
- W2931769884 cites W3100351867 @default.
- W2931769884 cites W3102050445 @default.
- W2931769884 cites W3102059530 @default.
- W2931769884 cites W3102579905 @default.
- W2931769884 cites W3103536668 @default.
- W2931769884 cites W3103642093 @default.
- W2931769884 cites W3103780616 @default.
- W2931769884 cites W3103836698 @default.
- W2931769884 cites W3104171173 @default.
- W2931769884 cites W3104972021 @default.
- W2931769884 cites W3105376889 @default.
- W2931769884 cites W3105550527 @default.
- W2931769884 cites W3106172690 @default.
- W2931769884 cites W3121278851 @default.
- W2931769884 cites W3124011327 @default.
- W2931769884 cites W4301383416 @default.
- W2931769884 doi "https://doi.org/10.3847/1538-4357/ab67bd" @default.
- W2931769884 hasPublicationYear "2020" @default.
- W2931769884 type Work @default.
- W2931769884 sameAs 2931769884 @default.
- W2931769884 citedByCount "24" @default.
- W2931769884 countsByYear W29317698842020 @default.
- W2931769884 countsByYear W29317698842021 @default.
- W2931769884 countsByYear W29317698842022 @default.
- W2931769884 countsByYear W29317698842023 @default.
- W2931769884 crossrefType "journal-article" @default.
- W2931769884 hasAuthorship W2931769884A5002705377 @default.
- W2931769884 hasAuthorship W2931769884A5007779776 @default.
- W2931769884 hasAuthorship W2931769884A5016187719 @default.
- W2931769884 hasAuthorship W2931769884A5039128270 @default.
- W2931769884 hasAuthorship W2931769884A5051825718 @default.
- W2931769884 hasAuthorship W2931769884A5080029324 @default.
- W2931769884 hasBestOaLocation W29317698841 @default.
- W2931769884 hasConcept C121332964 @default.
- W2931769884 hasConcept C124961601 @default.
- W2931769884 hasConcept C153294291 @default.
- W2931769884 hasConcept C178635117 @default.
- W2931769884 hasConcept C188721877 @default.
- W2931769884 hasConcept C198352243 @default.
- W2931769884 hasConcept C2524010 @default.
- W2931769884 hasConcept C33923547 @default.
- W2931769884 hasConcept C38652104 @default.
- W2931769884 hasConcept C41008148 @default.
- W2931769884 hasConcept C44870925 @default.
- W2931769884 hasConcept C63585750 @default.
- W2931769884 hasConcept C86132830 @default.
- W2931769884 hasConcept C98444146 @default.
- W2931769884 hasConceptScore W2931769884C121332964 @default.
- W2931769884 hasConceptScore W2931769884C124961601 @default.
- W2931769884 hasConceptScore W2931769884C153294291 @default.
- W2931769884 hasConceptScore W2931769884C178635117 @default.
- W2931769884 hasConceptScore W2931769884C188721877 @default.
- W2931769884 hasConceptScore W2931769884C198352243 @default.
- W2931769884 hasConceptScore W2931769884C2524010 @default.
- W2931769884 hasConceptScore W2931769884C33923547 @default.
- W2931769884 hasConceptScore W2931769884C38652104 @default.
- W2931769884 hasConceptScore W2931769884C41008148 @default.
- W2931769884 hasConceptScore W2931769884C44870925 @default.
- W2931769884 hasConceptScore W2931769884C63585750 @default.
- W2931769884 hasConceptScore W2931769884C86132830 @default.
- W2931769884 hasConceptScore W2931769884C98444146 @default.
- W2931769884 hasFunder F4320332623 @default.