activity
20172022
most citedA protostellar system fed by a streamer of 10,500 au length

166 citations · 806 across the 14 of their papers we have counts for

collaborators

19 papers

astro-ph.SR202130 cited

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…

astro-ph.GA20219 cited

No impact of core-scale magnetic field, turbulence, or velocity gradient on sizes of protostellar disks in Orion A

Hsi-Wei Yen, Bo Zhao, Patrick M. Koch +1

We compared the sizes and fluxes of a sample of protostellar disks in Orion A measured with the ALMA 0.87 mm continuum data from the VANDAM survey with the physical properties of t…

astro-ph.SR202139 cited

FAUST II. Discovery of a Secondary Outflow in IRAS 15398-3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?

Yuki Okoda, Yoko Oya, Logan Francis +66

We have observed the very low-mass Class 0 protostar IRAS 15398-3359 at scales ranging from 50 au to 1800 au, as part of the ALMA Large Program FAUST. We uncover a linear feature,…

astro-ph.SR202037 cited

Hall Effect in Protostellar Disc Formation and Evolution

Bo Zhao, Paola Caselli, Zhi-Yun Li +3

The Hall effect is recently shown to be efficient in magnetized dense molecular cores, and could lead to a bimodal formation of rotationally supported discs (RSDs) in the first cor…

astro-ph.GA2020166 cited

A protostellar system fed by a streamer of 10,500 au length

Jaime E. Pineda, Dominique Segura-Cox, Paola Caselli +5

Binary formation is an important aspect of star formation. One possible route for close-in binary formation is disk fragmentation. Recent observations show small scale…

astro-ph.GA202023 cited

Effect of grain size distribution and size-dependent grain heating on molecular abundances in starless and pre-stellar cores

O. Sipilä, B. Zhao, P. Caselli

We present a new gas-grain chemical model to constrain the effect of grain size distribution on molecular abundances in starless and pre-stellar cores. We introduce grain-size depe…