Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Eclipsing Systems with Pulsating Components (Types {\beta} Cep, {\delta}
  Sct, {\gamma} Dor or Red Giant) in the Era of High-Accuracy Space Data   Eclipsing systems are essential objects for understanding the properties of
stars and stellar systems. Eclipsing systems with pulsating components are
furthermore advantageous because they provide accurate constraints on the
component properties, as well as a complementary method for pulsation mode
determination, crucial for precise asteroseismology. The outcome of space
missions aiming at delivering high-accuracy light curves for many thousands of
stars in search of planetary systems has also generated new insights in the
field of variable stars and revived the interest of binary systems in general.
The detection of eclipsing systems with pulsating components has particularly
benefitted from this, and progress in this field is growing fast. In this
review, we showcase some of the recent results obtained from studies of
eclipsing systems with pulsating components based on data acquired by the space
missions {\it Kepler} or TESS. We consider different system configurations
including semi-detached eclipsing binaries in (near-)circular orbits, a
(near-)circular and non-synchronized eclipsing binary with a chemically
peculiar component, eclipsing binaries showing the heartbeat phenomenon, as
well as detached, eccentric double-lined systems. All display one or more
pulsating component(s). Among the great variety of known classes of pulsating
stars, we discuss unevolved or slightly evolved pulsators of spectral type B, A
or F and red giants with solar-like oscillations. Some systems exhibit
additional phenomena such as tidal effects, angular momentum transfer,
(occasional) mass transfer between the components and/or magnetic activity. How
these phenomena and the orbital changes affect the different types of
pulsations excited in one or more components, offers a new window of
opportunity to better understand the physics of pulsations.

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The categories of this paper are: nucl-ex
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The categories of this paper are: q-bio
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The categories of this paper are: math-ph
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The categories of this paper are: mtrl-th
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The categories of this paper are: hep-ex
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The categories of this paper are: gr-qc
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The categories of this paper are: cond-mat
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The categories of this paper are: hep-ph
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The categories of this paper are: q-alg
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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: math
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The categories of this paper are: adap-org
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The categories of this paper are: hep-th
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The categories of this paper are: dg-ga
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The categories of this paper are: funct-an