Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Resolved star formation in the metal poor star-forming region Magellanic
  Bridge C   Magellanic Bridge C (MB-C) is a metal-poor ($\sim$1/5 $Z_{\odot}$)
low-density star-forming region located 59 kpc away in the Magellanic Bridge,
offering a resolved view of the star formation process in conditions different
to the Galaxy. From Atacama Large Millimetre Array CO (1-0) observations, we
detect molecular clumps associated to candidate young stellar objects (YSOs),
pre-main sequence (PMS) stars, and filamentary structure identified in
far-infrared imaging. YSOs and PMS stars form in molecular gas having densities
between 17-200 $M_{\odot}$ pc$^{-2}$, and have ages between $\lesssim$0.1-3
Myr. YSO candidates in MB-C have lower extinction than their Galactic
counterparts. Otherwise, our results suggest that the properties and
morphologies of molecular clumps, YSOs, and PMS stars in MB-C present no patent
differences with respect to their Galactic counterparts, tentatively alluding
that the bottleneck to forming stars in regions similar to MB-C is the
conversion of atomic gas to molecular.

14
The categories of this paper are: math-ph
37
The categories of this paper are: supr-con
21
The categories of this paper are: adap-org
9
The categories of this paper are: nlin
34
The categories of this paper are: chem-ph
5
The categories of this paper are: gr-qc
7
The categories of this paper are: hep-th
33
The categories of this paper are: plasm-ph
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The categories of this paper are: q-fin
1
The categories of this paper are: cs
2
The categories of this paper are: math
26
The categories of this paper are: bayes-an
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The categories of this paper are: acc-phys
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The categories of this paper are: alg-geom
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The categories of this paper are: mtrl-th
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The categories of this paper are: nucl-th