Kavli Affiliate: David Charbonneau | First 5 Authors: Edward M. Bryant, Andrés Jordán, Joel D. Hartman, Daniel Bayliss, Elyar Sedaghati | Summary: Planet formation models suggest that the formation of giant planets is significantly harder around low-mass stars, due to the scaling of protoplanetary disc masses with stellar mass. The discovery of giant planets orbiting […]
Continue.. A transiting giant planet in orbit around a 0.2-solar-mass host star