Mass-To-Radius Profiles of Newtonian Polytropic Spheres: Low-Mass Main-Sequence Stars in Palatini Gravity Versus Dark-Matter-Admixed Low-Mass Stars in General Relativity

AuthID
 P-00Q-MYK
2
Author(s)
Document Type
Article
Year published
2019
Published
in PHYSICAL REVIEW D, ISSN: 2470-0010
Volume: 99, Issue: 10
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Publication Identifiers
Scopus: 2-s2.0-85066451107
Wos: WOS:000469024800002
Source Identifiers
ISSN: 2470-0010
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