30 citations · 54 across the 4 of their papers we have counts for
4 papers
Exploring the dust grain size and polarization mechanism in the hot and massive Class 0 disk IRAS 16293-2422 B
Joaquin Zamponi, María José Maureira, Hauyu Baobab Liu +4
Multiwavelength dust continuum and polarization observations arising from self-scattering have been used to investigate grain sizes in young disks. However, the polarization by sel…
Dust hot spots at 10 au scales around the Class 0 binary IRAS 16293-2422 A: a departure from the passive irradiation model
M. J. Maureira, M. Gong, J. E. Pineda +6
Characterizing the physical conditions at disk scales in Class 0 sources is crucial for constraining the protostellar accretion process and the initial conditions for planet format…
Synthetic observations using POLARIS: an application to simulations of massive prestellar cores
Joaquin Zamponi, Andrea Giannetti, Stefano Bovino +5
Young massive stars are usually found embedded in dense and massive molecular clumps which are known for being highly obscured and distant. During their formation process, the degr…
The young protostellar disk in IRAS16293-2422 B is hot and shows signatures of gravitational instability
Joaquin Zamponi, María José Maureira, Bo Zhao +4
Deeply embedded protostars are actively fed from their surrounding envelopes through their protostellar disk. The physical structure of such early disks might be different from tha…