Planetary-mass objects and brown dwarfs at the transition from relatively red L dwarfs to bluer mid-T dwarfs (Teff∼1300 K) show enhanced spectrophotometric variability.
Planetary-mass objects and brown dwarfs at the transition from relatively red L dwarfs to bluer mid-T dwarfs (Teff∼1300 K) show enhanced spectrophotometric variability.