activity
20222026
most citedCold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy

43 citations · 92 across the 11 of their papers we have counts for

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11 papers · 1 filter

astro-ph.GA2026

Anomalously high deuterium fractionation in a galactic translucent cloud: a challenge to chemical models

Gan Luo, Zhi-Yu Zhang, Thomas G. Bisbas +8

Deuterated (D-) species have long been proposed to diagnose the physical conditions and chemical evolution of cold dense molecular clouds. While deuterium fractionation has been ex…

astro-ph.GA2025★ 1 cited

Scientific Objectives of the Xue-shan-mu-chang 15-meter Submillimeter Telescope

XSMT Project Collaboration Group, Yiping Ao, Jin Chang +48

Submillimeter astronomy is poised to revolutionize our understanding of the Universe by revealing cosmic phenomena hidden from optical and near-infrared observations, particularly…

astro-ph.GA2025★ 6 cited

Inadequate turbulent support in low-metallicity molecular clouds

Lingrui Lin, Zhi-Yu Zhang, Junzhi Wang +16

The dynamic properties of molecular clouds are set by the interplay of their self-gravity, turbulence, external pressure and magnetic fields. Extended surveys of Galactic molecular…

astro-ph.GA2024★ 2 cited

Gas dynamics in an AGN-host galaxy at : regular rotation, non-circular motions, and mass models

Lingrui Lin, Federico Lelli, Carlos De Breuck +9

The gas dynamics of galaxies provide critical insights into the evolution of both baryons and dark matter (DM) across cosmic time. In this context, galaxies at cosmic noon -- the p…

astro-ph.GA2024

Molecular gas mass measurements of an active, starburst galaxy at using ALMA observations of the [CI], CO and dust emission

Hao-Tse Huang, Allison W. S. Man, Federico Lelli +7

We present new ALMA observations of a starburst galaxy at cosmic noon hosting a radio-loud active galactic nucleus: PKS 0529-549 at . To investigate the conditions of its c…

astro-ph.GA2024★ 10 cited

The CO-dark molecular gas in the cold HI arc

Gan Luo, Di Li, Zhi-yu Zhang +6

The CO-dark molecular gas (DMG), which refers to the molecular gas not traced by CO emission, is crucial for the evolution of the interstellar medium (ISM). While the gas propertie…