92 citations · 329 across the 6 of their papers we have counts for
13 papers
Resistive MHD Simulations of Star-Disk-Jet System
Miljenko Cemeljic, Hsien Shang, Tzu-Yang Chiang
Stellar magnetosphere and accretion disk interact, and a result should be outflow launched from the innermost vicinity of a protostellar object. We simulated physical conditions in…
First Confirmed Detection of a Bipolar Molecular Outflow from a Young Brown Dwarf
Ngoc Phan-Bao, Basmah Riaz, Chin-Fei Lee +6
Studying the earliest stages in the birth of stars is crucial for understanding how they form. Brown dwarfs with masses between that of stars and planets are not massive enough to…
X-winds in Action
Mike J. Cai, Hsien Shang, Hsiao-Hsuan Lin +1
The interaction of accretion disks with the magnetospheres of young stars can produce X-winds and funnel flows. With the assumption of axial symmetry and steady state flow, the pro…
Submillimeter arcsecond-resolution mapping of the highly collimated protostellar jet HH 211
Chin-Fei Lee, Paul T. P. Ho, Aina Palau +4
We have mapped the protostellar jet HH 211 in 342 GHz continuum, SiO (), and CO () emission at \arcs{1} resolution with the Submillimeter Array (SMA). Thermal…
A radiation driven implosion model for the enhanced luminosity of protostars near HII regions
K. Motoyama, T. Umemoto, H. Shang
Context. Molecular clouds near the H II regions tend to harbor more luminous protostars. Aims. Our aim in this paper is to investigate whether or not radiation-driven implosion mec…
HH 212: SMA Observations of a Remarkable Protostellar Jet
Chin-Fei Lee, Paul T. P. Ho, Henrik Beuther +4
HH 212 is a nearby (460 pc) protostellar jet discovered in H powered by a Class 0 source, IRAS 05413-0104, in the L1630 cloud of Orion. It is highly collimated and symmetric wi…