Skip to main content

Research Repository

Advanced Search

An Eddington-limited Accretion Disk Wind in the Narrow-line Seyfert 1 PG 1448+273

Reeves, J. N.; Braito, V.; Luminari, A.; Porquet, D.; Laurenti, M.; Matzeu, G.; Lobban, A.; Hagen, S.

An Eddington-limited Accretion Disk Wind in the Narrow-line Seyfert 1 PG 1448+273 Thumbnail


Authors

J. N. Reeves

V. Braito

A. Luminari

D. Porquet

M. Laurenti

G. Matzeu

A. Lobban

Profile image of Scott Hagen

Scott Hagen scott.hagen@durham.ac.uk
PGR Student Doctor of Philosophy



Abstract

PG 1448+273 is a luminous, nearby (z = 0.0645), narrow-line Seyfert 1 galaxy, which likely accretes close to the Eddington limit. Previous X-ray observations of PG 1448+273 with XMM-Newton in 2017 and NuSTAR in 2022 revealed the presence of an ultrafast outflow, as seen through its blueshifted iron (Fe) K absorption profile, where the outflow velocity appeared to vary in the range 0.1−0.3c. In this work, new X-ray observations of PG 1448+273 are presented, in the form of four simultaneous XMM-Newton and NuSTAR observations performed in 2023 July and August. The X-ray spectra appeared at a similar flux in each observation, making it possible to analyze the mean 2023 X-ray spectrum at high signal-to-noise ratio. A broad (σ = 1 keV) and highly blueshifted (E = 9.8 ± 0.4 keV) Fe K absorption profile is revealed in the mean spectrum. The profile can be modeled by a fast, geometrically thick accretion disk wind, which reveals a maximum terminal velocity of v ∞ = −0.43 ± 0.03c, one of the fastest known winds in a nearby active galactic nucleus. As a result, the inferred mass outflow rate of the wind may reach a significant fraction of the Eddington accretion rate.

Citation

Reeves, J. N., Braito, V., Luminari, A., Porquet, D., Laurenti, M., Matzeu, G., Lobban, A., & Hagen, S. (2024). An Eddington-limited Accretion Disk Wind in the Narrow-line Seyfert 1 PG 1448+273. The Astrophysical Journal, 974(1), Article 58. https://doi.org/10.3847/1538-4357/ad6b95

Journal Article Type Article
Acceptance Date Aug 4, 2024
Online Publication Date Oct 4, 2024
Publication Date Oct 1, 2024
Deposit Date Oct 21, 2024
Publicly Available Date Oct 21, 2024
Journal The Astrophysical Journal
Electronic ISSN 1538-4357
Peer Reviewed Peer Reviewed
Volume 974
Issue 1
Article Number 58
DOI https://doi.org/10.3847/1538-4357/ad6b95
Keywords High-luminosity active galactic nuclei, X-ray astronomy
Public URL https://durham-repository.worktribe.com/output/2956503

Files





You might also like



Downloadable Citations