000153025 001__ 153025 000153025 005__ 20251017144642.0 000153025 0247_ $$2doi$$a10.1016/j.physrep.2025.02.002 000153025 0248_ $$2sideral$$a143457 000153025 037__ $$aART-2025-143457 000153025 041__ $$aeng 000153025 100__ $$aCarenza, Pierluca 000153025 245__ $$aAxion astrophysics 000153025 260__ $$c2025 000153025 5060_ $$aAccess copy available to the general public$$fUnrestricted 000153025 5203_ $$aStars have been recognized as optimal laboratories to probe axion properties. In the last decades there have been significant advances in this field due to a better modeling of stellar systems and accurate observational data. In this work we review the current status of constraints on axions from stellar physics. We focus in particular on the Sun, globular cluster stars, white dwarfs and (proto)-neutron stars. 000153025 540__ $$9info:eu-repo/semantics/openAccess$$aAll rights reserved$$uhttp://www.europeana.eu/rights/rr-f/ 000153025 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/submittedVersion 000153025 700__ $$0(orcid)0000-0001-9823-6262$$aGiannotti, Maurizio$$uUniversidad de Zaragoza 000153025 700__ $$aIsern, Jordi 000153025 700__ $$aMirizzi, Alessandro 000153025 700__ $$aStraniero, Oscar 000153025 7102_ $$12004$$2038$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Astronomía y Astrofísica 000153025 773__ $$g1117 (2025), 1-102$$pPhys. rep.$$tPHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS$$x0370-1573 000153025 8564_ $$s7221250$$uhttps://zaguan.unizar.es/record/153025/files/texto_completo.pdf$$yPreprint 000153025 8564_ $$s1171058$$uhttps://zaguan.unizar.es/record/153025/files/texto_completo.jpg?subformat=icon$$xicon$$yPreprint 000153025 909CO $$ooai:zaguan.unizar.es:153025$$particulos$$pdriver 000153025 951__ $$a2025-10-17-14:32:38 000153025 980__ $$aARTICLE