Variability in a Young, L/T Transition Planetary-mass Object
As part of our ongoing NTT SoFI survey for variability in young free-floating planets and low-mass brown dwarfs, we detect significant variability in the young, free-floating planetary-mass object PSO J318.5–22, likely due to rotational modulation of inhomogeneous cloud cover. A member of the 23 ± 3 Myr β Pic moving group, PSO J318.5–22 has Teff =
Biller, B. A. et al.
Fecha de publicación:
11
2015