activity
20212024
most citedMeasuring Turbulence with Young Stars in the Orion Complex

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

collaborators

8 papers

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.HE2021★ 11 cited

Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations

Federico G. Lopez Armengol, Zachariah B. Etienne, Scott C. Noble +20

We perform binary neutron star (BNS) merger simulations in full dynamical general relativity with IllinoisGRMHD, on a Cartesian grid with adaptive-mesh refinement. After the remnan…

astro-ph.HE2021★ 25 cited

HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage

Ariadna Murguia-Berthier, Scott C. Noble, Luke F. Roberts +25

The first binary neutron star merger has already been detected in gravitational waves. The signal was accompanied by an electromagnetic counterpart including a kilonova component p…

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…