output
20062026
most citedA Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2

303 citations

Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026

Probing Dust Composition in Distant Galaxies with JWST Mid-IR Spectroscopy of Quasars with Foreground 2175 Å Absorbers II. Measurements of Grain Composition and Extinction Properties

Viacheslav V. Klimenko, Varsha P. Kulkarni, Monique C. Aller

We present results from a mini-survey of dust spectral features arising in galaxies at redshifts in our James Webb Space Telescope (JWST) mid-infrared spectra of ph…

astro-ph.GA2024

Metal-Poor Stars in the MW Disk: Resonant Cooling of Vertical Oscillations of Halo Stars in Barred Galaxies

Xingchen Li, Isaac Shlosman, Daniel Pfenniger +1

Using numerical simulations of barred disk galaxy embedded in nonspinning and spinning dark matter (DM) halos, we present a novel mechanism of `cooling' the vertical oscillations o…

astro-ph.GA2023

Evolution of Stellar Bars in Spinning Dark Matter Halos and Stellar Bulges

Xingchen Li, Isaac Shlosman, Daniel Pfenniger +1

We use high-resolution numerical simulations to follow the barred disk evolution in a suite of models with progressively more massive stellar bulges, with bulge-to-total (diskbu…

astro-ph.GA2022★ 18 cited

Stellar Bars in Spinning Halos: Delayed Buckling and Absence of Slowdown

Xingchen Li, Isaac Shlosman, Clayton Heller +1

We use high resolution numerical simulations in order to analyze the stellar bar evolution in spinning dark matter (DM) halos. Previous works have shown that the halo spin has a su…

astro-ph.GA2022★ 21 cited

The Origin of Buckling Instability in Galactic Bars: Searching for the Scapegoat

Xingchen Li, Isaac Shlosman, Daniel Pfenniger +1

The buckling process in stellar bars is full of unsolved issues. We analyze the origin of the buckling instability in stellar bars using high-resolution N-body simulations. Previou…

astro-ph.GA2020★ 20 cited

Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies

Bo Peng, Cody Lamarche, Gordon Stacey +8

The Nitrogen-to-Oxygen (N/O) abundance ratio is an important diagnostic of galaxy evolution since the ratio is closely tied to the growth of metallicity and the star formation hist…