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20022008
most citedSubmillimeter arcsecond-resolution mapping of the highly collimated protostellar jet HH 211

92 citations · 355 across the 6 of their papers we have counts for

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8 papers

astro-ph20089 cited

Infall and rotation motions in the HH 111 protostellar system: A flattened envelope in transition to a disk?

Chin-Fei Lee, Yao-Yuan Mao, Bo Reipurth

We have mapped the central region of the HH 111 protostellar system in 1.33 mm continuum, C18O(J=2-1), 13CO (J=2-1), and SO (N_J=5_6-4_5) emission at ~3" resolution with the Submil…

astro-ph200884 cited

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…

astro-ph200753 cited

The CO Molecular Outflows of IRAS 16293-2422 Probed by the Submillimeter Array

Sherry C. C. Yeh, Naomi Hirano, Tyler L. Bourke +4

We have mapped the proto-binary source IRAS 16293-2422 in CO 2-1, 13CO 2-1, and CO 3-2 with the Submillimeter Array (SMA). The maps with resolution of 1".5-5" reveal a single small…

astro-ph200792 cited

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…

astro-ph200791 cited

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…

astro-ph200626 cited

Molecular Outflows in Low- and High-Mass Star Forming Regions

Hector G. Arce, Debra Shepherd, Frederic Gueth +4

We review the known properties of molecular outflows from low- and high-mass young stars. General trends among outflows are identified, and the most recent studies on the morpholog…