Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Probing high-mass stellar evolutionary models with binary stars   Mass discrepancy is one of the problems that is pending a solution in
(massive) binary star research field. The problem is often solved by
introducing an additional near core mixing into evolutionary models, which
brings theoretical masses of individual stellar components into an agreement
with the dynamical ones. In the present study, we perform a detailed analysis
of two massive binary systems, V380 Cyg and Sigma Sco, to provide an
independent, asteroseismic measurement of the overshoot parameter, and to test
state-of-the-art stellar evolution models.

24
The categories of this paper are: dg-ga
30
The categories of this paper are: q-alg
1
The categories of this paper are: cs
33
The categories of this paper are: plasm-ph
10
The categories of this paper are: q-bio
29
The categories of this paper are: funct-an
22
The categories of this paper are: chao-dyn
17
The categories of this paper are: q-fin
34
The categories of this paper are: chem-ph
26
The categories of this paper are: bayes-an
9
The categories of this paper are: nlin
23
The categories of this paper are: solv-int
37
The categories of this paper are: supr-con
27
The categories of this paper are: comp-gas
7
The categories of this paper are: hep-th
20
The categories of this paper are: acc-phys