Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: The interplay between mass-loss and binarity   Most stars with birth masses larger than that of our Sun belong to binary or
higher order multiple systems. Similarly, most stars have stellar winds.
Radiation pressure and multiplicity create outflows of material that remove
mass from the primary star and inject it into the interstellar medium or
transfer it to a companion. Both have strong impact on the subsequent evolution
of the stars, yet they are often studied separately. In this short review, I
will sketch part of the landscape of the interplay between stellar winds and
binarity. I will present several examples where binarity shapes the stellar
outflows, providing new opportunities to understand and measure mass loss
properties. Stellar winds spectral signatures often help clearly identifying
key stages of stellar evolution. The multiplicity properties of these stages
then shed a new light onto evolutionary connections between the different
categories of evolved stars.

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The categories of this paper are: adap-org
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The categories of this paper are: nucl-ex
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The categories of this paper are: cmp-lg
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The categories of this paper are: cs
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The categories of this paper are: eess
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The categories of this paper are: patt-sol
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The categories of this paper are: chao-dyn
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The categories of this paper are: gr-qc
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The categories of this paper are: hep-th
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The categories of this paper are: chem-ph
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The categories of this paper are: alg-geom
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The categories of this paper are: nlin
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The categories of this paper are: hep-lat
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The categories of this paper are: cond-mat
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The categories of this paper are: comp-gas
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The categories of this paper are: nucl-th