Confirmed observations of young protoplanets actively undergoing the process of formation have remained rare to date. In this Letter, we present new insights into the nature of the recently identified protoplanet WISPIT 2 b (age $\sim$ 5 Myr) from VLTI/GRAVITY+ observations. Through the analysis of the spectral energy...
G. Collaboration, K. A. El Dayem, R. Abuter et al.· 1 citation
The formation mechanisms of brown dwarfs (BDs) and free-floating planets (FFPs) are poorly constrained. The two main competing scenarios include the star-like scenario, where these objects correspond to the least massive gravitationally unstable fragments of molecular clouds, and the planet-like scenario, where these o...
A. Palau, D. Stamatellos, M. Bate et al.· 0 citations
Giant planets are often regarded as primordial protoplanetary"architects". Their formation and interactions with planetesimals and other planets during and after the protoplanetary disc phase are key to setting the blueprint of the planetary systems we observe today. Catching nascent gas giants is our best opportunity...
F. Zagaria, A. Izquierdo, J. Bae et al.· 0 citations
Kinematic perturbations observed with the Atacama Large Millimeter/submillimeter Array in CO line emission provide evidence for a population of embedded giant protoplanets shaping the structure of protoplanetary disks. We present JWST/MIRI F1140C (λ = 11.3 μm) coronagraphic observations of five protoplanetary disks—HD...
G. Cugno, M. Benisty, R. Teague et al.· Astronomical Journal· 0 citations
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