Meta-modelling the climate of dry tide-locked rocky planets - HAL
Terrestrial planets orbiting within the habitable zones of M-stars are likely to become tidally locked in a 1:1 spin: orbit configuration and ...
Prospects for the characterization of habitable planetsMost planets located in the habitable zone of sub-Solar- mass stars, and particularly those orbiting very-low-mass dwarfs such as TRAPPIST-1, ... CLIMATE INSTABILITY ON TIDALLY LOCKED EXOPLANETSFor planets in the middle and outer ranges of the habitable zone, the possibility of hurricane formation is low or even close to zero, as has been suggested in ... Atmospheric stability and collapse on tidally locked rocky planetsTidally locked worlds provide a unique opportunity for constraining the probable climates of certain exoplanets. They are unique.
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