Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Planet Formation Around M-dwarfs: From Young Disks to Planets   Cool M dwarfs outnumber sun-like G stars by ten to one in the solar
neighborhood. Due to their proximity, small size, and low mass, M-dwarf stars
are becoming attractive targets for exoplanet searches via almost all current
search methods. But what planetary systems can form around M dwarfs? Following
up on the Cool Stars~16 Splinter Session "Planet Formation Around M Dwarfs", we
summarize here our knowledge of protoplanetary disks around cool stars, how
they disperse, what planetary systems might form and can be detected with
current and future instruments.

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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: hep-ex
17
The categories of this paper are: q-fin
31
The categories of this paper are: ao-sci
27
The categories of this paper are: comp-gas
32
The categories of this paper are: atom-ph
9
The categories of this paper are: nlin
5
The categories of this paper are: gr-qc
29
The categories of this paper are: funct-an
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The categories of this paper are: cs
26
The categories of this paper are: bayes-an
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The categories of this paper are: cmp-lg
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The categories of this paper are: math
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The categories of this paper are: nucl-ex
18
The categories of this paper are: econ