activity
20152021
most citedDust masses of young disks: constraining the initial solid reservoir for planet formation

204 citations · 236 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.GA20212 cited

Imaging the water snowline around protostars with water and HCO isotopologues

Merel L. R. van 't Hoff, Daniel Harsono, Martijn L. van Gelder +7

The water snowline location in protostellar envelopes provides crucial information about the thermal structure and the mass accretion process as it can inform about the occurrence…

astro-ph.GA2021

K-band High-Resolution Spectroscopy of Embedded Massive Protostars

Tien-Hao Hsieh, Michihiro Takami, Michael S. Connelley +7

A classical paradox in high-mass star formation is that powerful radiation pressure can halt accretion, preventing further growth of a central star. Disk accretion has been propose…

gr-qc2021

Strong gravitational lensing by Kerr and Kerr-Newman black holes

Tien Hsieh, Da-Shin Lee, Chi-Yong Lin

We study the strong gravitational lensing due to the Kerr black holes with angular momentum and the Kerr-Newman black holes with additional charge . We first derive the anal…

astro-ph.SR202016 cited

Multi-epoch SMA observations of the L1448C(N) protostellar SiO jet

Tomohiro Yoshida, Tien-Hao Hsieh, Naomi Hirano +1

L1448C(N) is a young protostar in Perseus, driving an outflow and an extremely high-velocity (EHV) molecular jet. We present multi-epoch observations of SiO , CO

astro-ph.EP2020204 cited

Dust masses of young disks: constraining the initial solid reservoir for planet formation

Łukasz Tychoniec, Carlo F. Manara, Giovanni P. Rosotti +7

In recent years evidence has been building that planet formation starts early, in the first 0.5 Myr. Studying the dust masses available in young disks enables understanding…

astro-ph.SR2019

An ALMA Study of the FU-Ori Type Object V900 Mon: Implications for the Progenitor

Michihiro Takami, Tsu-Sheng Chen, Hauyu Baobab Liu +13

We present ALMA observations of 12CO, 13CO, and C18O J=2--1 lines and the 230 GHz continuum for the FU Ori-type object (FUor) V900 Mon (d~1.5 kpc), for which the accretion burst wa…