The demographic of circumstellar disks, the birthplaces of planets, is diverse and rich in disks featuring rings, gaps, spirals, filaments, and arcs. Many studies revealing these disk …
R Dong, S Liu, J Eisner, S Andrews… - The Astrophysical …, 2018 - iopscience.iop.org
Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a …
J Huang, EA Bergin, KI Öberg… - The Astrophysical …, 2021 - iopscience.iop.org
The concentric gaps and rings commonly observed in protoplanetary disks in millimeter continuum emission have lent the impression that planet formation generally proceeds …
Close encounters between young stellar objects in star-forming clusters are expected to markedly perturb circumstellar disks. Such events are witnessed in numerical simulations of …
Deciphering the spatial and temporal evolution of chondrules allows for a better understanding of how asteroidal seeds formed, migrated, and eventually accreted into …
J Huang, EA Bergin, J Bae, M Benisty… - The Astrophysical …, 2023 - iopscience.iop.org
DR Tau has been noted for its unusually high variability in comparison with other T Tauri stars. Although it is one of the most extensively studied pre-main-sequence stars …
R Dong, JR Najita, S Brittain - The Astrophysical Journal, 2018 - iopscience.iop.org
Spiral arm structures seen in scattered-light observations of protoplanetary disks can potentially serve as signposts of planetary companions. They can also lend unique insights …
We investigate the formation of protoplanetary disks around nine solar-mass stars formed in the context of a (40 pc) 3 Giant Molecular Cloud model, using ramses adaptive mesh …
TH Hsieh, NM Murillo, A Belloche… - The Astrophysical …, 2019 - iopscience.iop.org
Episodic accretion has been used to explain the wide range of protostellar luminosities, but its origin and influence on the star-forming process are not yet fully understood. We present …