Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Mass-radius relations for white dwarf stars of different internal
  compositions   The purpose of this work is to present accurate and detailed mass-radius
relations for white dwarf (WD) models with helium, carbon, oxygen, silicon and
iron cores, by using a fully updated stellar evolutionary code. We considered
masses from 0.15 to 0.5 Mo for the case of helium core, from 0.45 to 1.2 Mo for
carbon, oxygen and silicon cores and from 0.45 to 1.0 Mo for the case of an
iron core. In view of recent measurements made by Hipparcos that strongly
suggest the existence of WDs with an iron-dominated core, we focus our
attention mainly on the finite-temperature, mass-radius relations for WD models
with iron interiors. Furthermore, we explore the effects of gravitational,
chemical and thermal diffusion on low-mass helium WD models with hydrogen and
helium envelopes.

28
The categories of this paper are: alg-geom
2
The categories of this paper are: math
22
The categories of this paper are: chao-dyn
7
The categories of this paper are: hep-th
17
The categories of this paper are: q-fin
3
The categories of this paper are: physics
15
The categories of this paper are: nucl-ex
31
The categories of this paper are: ao-sci
14
The categories of this paper are: math-ph
25
The categories of this paper are: patt-sol
8
The categories of this paper are: hep-ex
21
The categories of this paper are: adap-org
35
The categories of this paper are: mtrl-th
18
The categories of this paper are: econ
9
The categories of this paper are: nlin
36
The categories of this paper are: cmp-lg