Host star metallicity of directly imaged wide-orbit planets: implications for planet formation

C. Swastik, Ravinder K. Banyal, Mayank Narang +4

Directly imaged planets are self-luminous companions of pre-main sequence and young main sequence stars. They reside in wider orbits ($\sim 10\mathrm{s}-1000\mathrm{s}$~AU) and gene…