Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation

J. Maldonado, G. M. Mirouh, I. Mendigutía +3

The number of known planets around intermediate-mass stars (1.5 M${}_{\odot }$ < M${}_{\star }$ < 3.5 M${}_{\odot }$) is rather low. We aim to test whether the correlation between the metal…