Matches in SemOpenAlex for { <https://semopenalex.org/work/W2129208047> ?p ?o ?g. }
- W2129208047 endingPage "27" @default.
- W2129208047 startingPage "1" @default.
- W2129208047 abstract "Context. AGN outflows are thought to influence the evolution of their host galaxies and of super massive black holes. Our deep multiwavelength campaign on NGC 5548 has revealed a new, unusually strong X-ray obscuration, accompanied by broad UV absorption troughs observed for the first time in this object. The X-ray obscuration caused a dramatic decrease in the incident ionizing flux on the outflow that produces the long-studied narrow UV absorption lines in this AGN. The resulting data allowed us to construct a comprehensive physical, spatial, and temporal picture for this enduring AGN wind.Aims. We aim to determine the distance of the narrow UV outflow components from the central source, their total column-density, and the mechanism responsible for their observed absorption variability.Methods. We study the UV spectra acquired during the campaign, as well as from four previous epochs (1998−2011). Our main analysis tools are ionic column-density extraction techniques, photoionization models based on the code CLOUDY, and collisional excitation simulations.Results. A simple model based on a fixed total column-density absorber, reacting to changes in ionizing illumination, matches the very different ionization states seen in five spectroscopic epochs spanning 16 years. The main component of the enduring outflow is situated at 3.5 ± 1.1 pc from the central source, and its distance and number density are similar to those of the narrow-emitting-line region in this object. Three other components are situated between 5−70 pc and two are farther than 100 pc. The wealth of observational constraints and the anti-correlation between the observed X-ray and UV flux in the 2002 and 2013 epochs make our physical model a leading contender for interpreting trough variability data of quasar outflows.Conclusions. This campaign, in combination with prior UV and X-ray data, yields the first simple model that can explain the physical characteristics and the substantial variability observed in an AGN outflow." @default.
- W2129208047 created "2016-06-24" @default.
- W2129208047 creator A5002902927 @default.
- W2129208047 creator A5005418936 @default.
- W2129208047 creator A5007006031 @default.
- W2129208047 creator A5008070377 @default.
- W2129208047 creator A5010587713 @default.
- W2129208047 creator A5015838280 @default.
- W2129208047 creator A5020299088 @default.
- W2129208047 creator A5020656183 @default.
- W2129208047 creator A5022157558 @default.
- W2129208047 creator A5023022205 @default.
- W2129208047 creator A5026031896 @default.
- W2129208047 creator A5027255654 @default.
- W2129208047 creator A5028769516 @default.
- W2129208047 creator A5031917607 @default.
- W2129208047 creator A5032322585 @default.
- W2129208047 creator A5032520367 @default.
- W2129208047 creator A5034390983 @default.
- W2129208047 creator A5044156949 @default.
- W2129208047 creator A5051273204 @default.
- W2129208047 creator A5054158025 @default.
- W2129208047 creator A5067527869 @default.
- W2129208047 creator A5068988311 @default.
- W2129208047 creator A5072665080 @default.
- W2129208047 creator A5076236404 @default.
- W2129208047 creator A5076442584 @default.
- W2129208047 creator A5077003465 @default.
- W2129208047 creator A5082652920 @default.
- W2129208047 creator A5082880965 @default.
- W2129208047 creator A5085177688 @default.
- W2129208047 creator A5087678090 @default.
- W2129208047 creator A5088511417 @default.
- W2129208047 creator A5090338092 @default.
- W2129208047 creator A5091303690 @default.
- W2129208047 date "2015-05-01" @default.
- W2129208047 modified "2023-10-15" @default.
- W2129208047 title "Anatomy of the AGN in NGC 5548 - II. The spatial, temporal, and physical nature of the outflow from HST/COS Observations" @default.
- W2129208047 cites W1516675624 @default.
- W2129208047 cites W1623597866 @default.
- W2129208047 cites W1969439547 @default.
- W2129208047 cites W1972615891 @default.
- W2129208047 cites W1977604962 @default.
- W2129208047 cites W1981107066 @default.
- W2129208047 cites W1989432205 @default.
- W2129208047 cites W2001872772 @default.
- W2129208047 cites W2002983479 @default.
- W2129208047 cites W2009228199 @default.
- W2129208047 cites W2009488872 @default.
- W2129208047 cites W2029343094 @default.
- W2129208047 cites W2035495564 @default.
- W2129208047 cites W2045875481 @default.
- W2129208047 cites W2046722348 @default.
- W2129208047 cites W2057953757 @default.
- W2129208047 cites W2059634633 @default.
- W2129208047 cites W2073838033 @default.
- W2129208047 cites W2073906329 @default.
- W2129208047 cites W2074620144 @default.
- W2129208047 cites W2081240894 @default.
- W2129208047 cites W2090270187 @default.
- W2129208047 cites W2100540266 @default.
- W2129208047 cites W2111034396 @default.
- W2129208047 cites W2114085446 @default.
- W2129208047 cites W2140557998 @default.
- W2129208047 cites W2141846043 @default.
- W2129208047 cites W2142993354 @default.
- W2129208047 cites W2169522826 @default.
- W2129208047 cites W2599691642 @default.
- W2129208047 cites W2762265283 @default.
- W2129208047 cites W3099512977 @default.
- W2129208047 cites W3101449570 @default.
- W2129208047 cites W3104779861 @default.
- W2129208047 cites W3104990928 @default.
- W2129208047 cites W3105389673 @default.
- W2129208047 cites W3105953634 @default.
- W2129208047 cites W3124410100 @default.
- W2129208047 hasPublicationYear "2015" @default.
- W2129208047 type Work @default.
- W2129208047 sameAs 2129208047 @default.
- W2129208047 citedByCount "10" @default.
- W2129208047 countsByYear W21292080472015 @default.
- W2129208047 countsByYear W21292080472016 @default.
- W2129208047 countsByYear W21292080472017 @default.
- W2129208047 countsByYear W21292080472021 @default.
- W2129208047 crossrefType "journal-article" @default.
- W2129208047 hasAuthorship W2129208047A5002902927 @default.
- W2129208047 hasAuthorship W2129208047A5005418936 @default.
- W2129208047 hasAuthorship W2129208047A5007006031 @default.
- W2129208047 hasAuthorship W2129208047A5008070377 @default.
- W2129208047 hasAuthorship W2129208047A5010587713 @default.
- W2129208047 hasAuthorship W2129208047A5015838280 @default.
- W2129208047 hasAuthorship W2129208047A5020299088 @default.
- W2129208047 hasAuthorship W2129208047A5020656183 @default.
- W2129208047 hasAuthorship W2129208047A5022157558 @default.
- W2129208047 hasAuthorship W2129208047A5023022205 @default.
- W2129208047 hasAuthorship W2129208047A5026031896 @default.
- W2129208047 hasAuthorship W2129208047A5027255654 @default.
- W2129208047 hasAuthorship W2129208047A5028769516 @default.