@article{
 title = {CHEERS Results from NGC 3393, II: Investigating the Extended Narrow Line Region using Deep Chandra Observations and Hubble Narrow Line Imaging},
 type = {article},
 year = {2016},
 identifiers = {[object Object]},
 websites = {http://arxiv.org/abs/1611.05880},
 id = {70b1e5d9-659b-3f82-8bed-7d009c10f15a},
 created = {2017-03-16T21:22:56.256Z},
 accessed = {2017-03-16},
 file_attached = {true},
 profile_id = {d9ca9665-cda3-3617-b3e8-ecfc7a8d9739},
 group_id = {5a95a0b6-1946-397c-b16a-114c6fdf3127},
 last_modified = {2017-03-27T20:34:50.654Z},
 read = {false},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {false},
 citation_key = {Maksym},
 private_publication = {false},
 abstract = {The CHandra Extended Emission Line Region Survey (CHEERS) is an X-ray study of nearby active galactic nuclei (AGN) designed to take full advantage of Chandra's unique angular resolution by spatially resolving feedback signatures and effects. In the second paper of a series on CHEERS target NGC 3393, we examine deep high-resolution Chandra images and compare them with Hubble narrow line images of [O III], [S II] and H$\alpha$, as well as previously-unpublished mid-ultraviolet (MUV) images. We find evidence for a complex multi-phase structure in the circumnuclear ISM, with no single simple correlation between X-rays and high-ionization ([O III]/H$\alpha$-dominated) and low-ionization ([S II]-dominated) features. We also find X-ray structures ~50-pc in extent, H$\alpha$ evidence for gas compression, and extended MUV emission associated with the S-shaped arms that envelope the radio jets. In conjunction with existing STIS kinematics, these findings support a role for shock contributions to the feedback, driven by the radio outflows associated with the radio jets.},
 bibtype = {article},
 author = {Maksym, W. Peter and Fabbiano, Giuseppina and Elvis, Martin and Karovska, Margarita and Paggi, Alessandro and Raymond, John and Wang, Junfeng and Storchi-Bergmann, Thaisa}
}

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