TY  - GEN 
AU  - Maldonado, Jesús
AU  - Mirouh, Giovanni Marcello
AU  - Mendigutía, Ignacio
AU  - Montesinos, Benjamin
AU  - Gragera-Más, José Luis
AU  - Villaver, Eva
PY  - 2025
UR  - https://hdl.handle.net/10481/111734
AB  - Context. Currently, the number of known planets around intermediate-mass stars (1.5 M⊙ < M⋆ < 3.5 M⊙) is rather low. As a consequence, models of planet formation derive their strongest observational evidence from the chemical signature of mostly...
LA  - eng
PB  - EDP Sciences
KW  - techniques: spectroscopic
KW  - planets and satellites: formation
KW  - stars: abundances
KW  - stars: early-type
KW  - Solar and Stellar Astrophysics
KW  - Earth and Planetary Astrophysics
TI  - Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation
DO  - 10.1051/0004-6361/202453328
ER  -