103 citations · 251 across the 20 of their papers we have counts for
6 papers · 1 filter
Early Planet Formation in Embedded Disks (eDisk) XXII: Keplerian disk, disk structures and jets/outflows in the Class 0 protostar IRAS 04166+2706
Nguyen Thi Phuong, Chang Won Lee, John J. Tobin +20
We present ALMA observations of the Class 0 protostar IRAS 04166+2706, obtained as part of the ALMA large program Early Planet Formation in Embedded Disks (eDisk). These observatio…
Early Grain Growth in the Young Protostellar Disk HH 212 Supported by Dust Self-Scattering Modeling
Ying-Chi Hu, Chin-Fei Lee, Zhe-Yu Daniel Lin +3
Grain growth in disks around young stars plays a crucial role in the formation of planets. Early grain growth has been suggested in the HH 212 protostellar disk by previous polariz…
Multiple misaligned outflows and warped accretion flows in the proto-multiple system Per-emb-8 and 55
Shang-Jing Lin, Hsi-Wei Yen, Shih-Ping Lai
To investigate the formation process of multiple systems, we have analyzed the ALMA archival data of the 1.3 mm continuum, CO (2-1) and CO (2-1) emission in a proto-m…
The First Estimation of the Ambipolar Diffusivity Coefficient from Multi-Scale Observations of the Class 0/I Protostar, HOPS-370
Travis J. Thieme, Shih-Ping Lai, Yueh-Ning Lee +2
Protostars are born in magnetized environments. As a consequence, the formation of protostellar disks can be suppressed by the magnetic field efficiently removing angular momentum…
Resolving Linear Polarization due to Emission and Extinction of Aligned Dust Grains on NGC1333 IRAS4A with JVLA and ALMA
Chia-Lin Ko, Hauyu Baobab Liu, Shih-Ping Lai +3
We report high angular resolution observations of linearly polarized dust emission towards the Class 0 young stellar object (YSO) NGC1333 IRAS4A (hereafter, IRAS4A) using the Karl…
Helical Magnetic Fields in the NGC1333 IRAS 4A Protostellar Outflows
Tao-Chung Ching, Shih-Ping Lai, Qizhou Zhang +3
We present Submillimeter Array (SMA) polarization observations of the CO = 3--2 line toward the NGC1333 IRAS 4A. The CO Stokes maps at an angular resolution of 1$\arc…