Constraining the geometry of the nuclear wind in PDS456 using a novel emission model

Outflows from AGNs are a key ingredient in the framework of feedback and coevolution with the host galaxy. In order to constrain the properties and evaluate the impact of the outflows, it is necessary to model their geometry and kinematics from accretion disk up to galaxy-scales. WINE (WINd Emission) is a Monte Carlo model to simulate geometry and kinematics, and estimate the associated emission line profiles, from the X-ray up to the infrared. We hereby present its features as well as its application to the Ultra Fast Outflow (UFO) in the quasar PDS456, a rosetta stone for studying nuclear winds. We also illustrate further developments currently undergoing.

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PID https://www.doi.org/10.5281/zenodo.1472693
PID https://www.doi.org/10.5281/zenodo.1472694
URL http://dx.doi.org/10.5281/zenodo.1472694
URL https://zenodo.org/record/1472694
URL http://dx.doi.org/10.5281/zenodo.1472693
URL https://figshare.com/articles/Constraining_the_geometry_of_the_nuclear_wind_in_PDS456_using_a_novel_emission_model/7263566
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Access Right Open Access
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Author Luminari, Alfredo
Author Piconcelli, E.
Author Tombesi, F.
Author Zappacosta, L.
Author Fiore, F.
Author Piro, L.
Author Vagnetti, F.
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Collected From ZENODO; figshare; Datacite; FigShare
Hosted By Zenodo; ZENODO; figshare; FigShare
Publication Date 2018-10-26
Additional Info
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Language Undetermined
Resource Type Other literature type; Conference object
keyword X-rays: galaxies
keyword galaxies: active
keyword line: profiles
keyword techniques: spectroscopic
keyword quasars: supermassive black holes
keyword quasars: emission lines
keyword arxiv.Astrophysics::Solar and Stellar Astrophysics
keyword arxiv.Astrophysics::Cosmology and Extragalactic Astrophysics
keyword arxiv.Astrophysics::High Energy Astrophysical Phenomena
keyword arxiv.Astrophysics::Galaxy Astrophysics
system:type publication
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Source https://science-innovation-policy.openaire.eu/search/publication?articleId=dedup_wf_001::d1b0f1186f8bbd581fe8950f3d8c85e7
Author jsonws_user
Last Updated 26 December 2020, 22:23 (CET)
Created 26 December 2020, 22:23 (CET)