activity
20182022
most citedAnomalously low metallicity regions in MaNGA star-forming galaxies: Accretion Caught in Action?

54 citations · 235 across the 8 of their papers we have counts for

collaborators

15 papers

astro-ph.SR202216 cited

Enhancement of Double-Close-Binary Quadruples

Gavin B. Fezenko, Hsiang-Chih Hwang, Nadia L. Zakamska

Double-close-binary quadruples (2+2 systems) are hierarchical systems of four stars where two short-period binary systems move around their common center of mass on a wider orbit.…

astro-ph.GA2021

A hidden population of high-redshift double quasars unveiled by astrometry

Yue Shen, Yu-Ching Chen, Hsiang-Chih Hwang +6

Galaxy mergers occur frequently in the early universe and bring multiple supermassive black holes (SMBHs) into the nucleus, where they may eventually coalesce. Identifying post-mer…

astro-ph.GA202023 cited

Evidence for the Accretion of Gas in Star-Forming Galaxies: High N/O Abundances in Regions of Anomalously-Low Metallicity

Yuanze Luo, Timothy Heckman, Hsiang-Chih Hwang +11

While all models for the evolution of galaxies require the accretion of gas to sustain their growth via on-going star formation, it has proven difficult to directly detect this inf…

astro-ph.SR202026 cited

Variability, periodicity and contact binaries in WISE

Evan Petrosky, Hsiang-Chih Hwang, Nadia L. Zakamska +2

The time-series component of WISE is a valuable resource for the study of variable objects. We present an analysis of an all-sky sample of ~450,000 AllWISE+NEOWISE infrared light c…

astro-ph.SR2020

The non-monotonic, strong metallicity dependence of the wide-binary fraction

Hsiang-Chih Hwang, Yuan-Sen Ting, Kevin C. Schlaufman +2

The metallicity dependence of the wide-binary fraction in stellar populations plays a critical role in resolving the open question of wide binary formation. In this paper, we inves…

astro-ph.SR202034 cited

A Gravitational Redshift Measurement of the White Dwarf Mass-Radius Relation

Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska +1

The mass-radius relation of white dwarfs is largely determined by the equation of state of degenerate electrons, which causes the stellar radius to decrease as mass increases. Here…