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Journal Article

The Close AGN Reference Survey (CARS). No evidence of galaxy-scale hot outflows in two nearby AGN

MPS-Authors

Powell,  M. C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Husemann,  B.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tremblay,  G. R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Krumpe,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Urrutia,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Baum,  S. A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Busch,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Combes,  F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Croom,  S. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Davis,  T. A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Eckart,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

O'Dea,  C. P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pérez-Torres,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Scharwächter,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Smirnova-Pinchukova,  I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Urry,  C. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018A&A...618A..27P
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Citation

Powell, M. C., Husemann, B., Tremblay, G. R., Krumpe, M., Urrutia, T., Baum, S. A., et al. (2018). The Close AGN Reference Survey (CARS). No evidence of galaxy-scale hot outflows in two nearby AGN. Astronomy and Astrophysics, 618.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CBA8-9
Abstract

Aims: We probe the radiatively-efficient, hot wind feedback mode in two nearby luminous unobscured (type 1) AGN from the Close AGN Reference Survey (CARS), which show intriguing kpc-scale arc-like features of extended [O III]ionized gas as mapped with VLT-MUSE. We aimed to detect hot gas bubbles that would indicate the existence of powerful, galaxy-scale outflows in our targets, HE 0227-0931 and HE 0351+0240, from deep (200 ks) Chandra observations.
Methods: By measuring the spatial and spectral properties of the extended X-ray emission and comparing with the sub kpc-scale IFU data, we are able to constrain feedback scenarios and directly test if the ionized gas is due to a shocked wind.
Results: No extended hot gas emission on kpc- scales was detected. Unless the ambient medium density is low (n H ̃ 1 cm-3 at 100 pc), the inferred upper limits on the extended X-ray luminosities are well below what is expected from theoretical models at matching AGN luminosities.
Conclusions: We conclude that the highly-ionized gas structures on kpc scales are not inflated by a hot outflow in either target, and instead are likely caused by photoionization of pre-existing gas streams of different origins. Our nondetections suggest that extended X-ray emission from an AGN-driven wind is not universal, and may lead to conflicts with current theoretical predictions. The scientific results reported in this article are based on observations made by the Chandra X-ray Observatory (PI: G. Tremblay, ID: 17700519), and on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere under ESO program(s) 094.B-0345(A) (PI: B. Husemann).