Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: MAGNUM survey: A MUSE-Chandra resolved view on ionized outflows and
  photoionization in the Seyfert galaxy NGC 1365   Ionized outflows, revealed by broad asymmetric wings of the [OIII] line, are
commonly observed in AGN but the low intrinsic spatial resolution of
observations has generally prevented a detailed characterization of their
properties. The MAGNUM survey aims at overcoming these limitations by focusing
on the nearest AGN, including NGC 1365, a nearby Seyfert galaxy (D~17 Mpc),
hosting a low-luminosity AGN (Lbol ~ 2x10^43 erg/s). We want to obtain a
detailed picture of the ionized gas in the central ~5 kpc of NGC 1365 in terms
of physical properties, kinematics, and ionization mechanisms. We also aim to
characterize the warm ionized outflow as a function of distance from the
nucleus and its relation with the nuclear X-ray wind. We employed VLT/MUSE
optical integral field spectroscopic observations to investigate the warm
ionized gas and Chandra ACIS-S X-ray data for the hot highly-ionized phase. We
obtained flux, kinematic, and diagnostic maps of the optical emission lines,
which we used to disentangle outflows from disk motions and measure the gas
properties down to a spatial resolution of ~70 pc. [OIII] emission mostly
traces an AGN-ionized kpc-scale biconical outflow with velocities up to ~200
km/s. H{\alpha} emission traces instead star formation in a circumnuclear ring
and along the bar, where we detect non-circular motions. Soft X-rays are mostly
due to thermal emission from the star-forming regions, but we could isolate the
AGN photoionized component which matches the [OIII] emission. The mass outflow
rate of the extended ionized outflow matches that of the nuclear X-ray wind and
then decreases with radius. However, the hard X-ray emission from the
circumnuclear ring suggests that star formation might contribute to the
outflow. The integrated mass outflow rate, kinetic energy rate, and outflow
velocity are broadly consistent with the typical relations observed in more
luminous AGN.

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The categories of this paper are: q-bio
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The categories of this paper are: hep-lat
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The categories of this paper are: eess
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The categories of this paper are: hep-th
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The categories of this paper are: atom-ph
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The categories of this paper are: chao-dyn
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The categories of this paper are: ao-sci
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The categories of this paper are: econ
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The categories of this paper are: solv-int
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The categories of this paper are: funct-an
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The categories of this paper are: adap-org
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The categories of this paper are: supr-con
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The categories of this paper are: cmp-lg
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The categories of this paper are: nucl-th
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The categories of this paper are: acc-phys
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The categories of this paper are: gr-qc