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20212024
most citedMeasuring Turbulence with Young Stars in the Orion Complex

35 citations · 120 across the 8 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2024

Rest-Frame Optical Spectroscopy of Ten z 2 Weak Emission-Line Quasars

Ying Chen, Bin Luo, W. N. Brandt +7

We present near-infrared spectroscopy of ten weak emission-line quasars (WLQs) at redshifts of , obtained with the Palomar 200-inch Hale Telescope. WLQs are an exceptional…

astro-ph.GA2024

Gemini Near Infrared Spectrograph -- Distant Quasar Survey: Rest-Frame Ultraviolet-Optical Spectral Properties of Broad Absorption Line Quasars

Harum Ahmed, Ohad Shemmer, Brandon Matthews +12

We present the rest-frame ultraviolet-optical spectral properties of 65 broad absorption line (BAL) quasars from the Gemini Near Infrared Spectrograph-Distant Quasar Survey (GNIRS-…

astro-ph.GA2023★ 2 cited

The Nature of the Motions of Multiphase Filaments in the Centers of Galaxy Clusters

Shalini Ganguly, Yuan Li, Valeria Olivares +6

The intracluster medium (ICM) in the centers of galaxy clusters is heavily influenced by the ``feedback'' from supermassive black holes (SMBHs). Feedback can drive turbulence in th…

astro-ph.GA2023★ 13 cited

Shedding New Light on Weak Emission-Line Quasars in the C-H Parameter Space

Trung Ha, Cooper Dix, Brandon M. Matthews +20

Weak emission-line quasars (WLQs) are a subset of Type 1 quasars that exhibit extremely weak LyN V 1240 and/or C IV 1549 emission lines. We investigate the relationship b…

astro-ph.GA2022★ 34 cited

Turbulence in Milky Way Star-Forming Regions Traced by Young Stars and Gas

Trung Ha, Yuan Li, Marina Kounkel +3

The interstellar medium (ISM) is turbulent on all scales and in all phases. In this paper, we study turbulence with different tracers in four nearby star-forming regions: Orion, Op…

astro-ph.GA2021★ 35 cited

Measuring Turbulence with Young Stars in the Orion Complex

Trung Ha, Yuan Li, Siyao Xu +2

Stars form in molecular clouds in the interstellar medium (ISM) with a turbulent kinematic state. Newborn stars therefore should retain the turbulent kinematics of their natal clou…