collaborators

6 papers

astro-ph.GA2026

Post-starburst Galaxies with Active Galactic Nucleus: Properties and Evolutionary Sequences

Junjie Huang, Yanmei Chen, Yong Shi +7

Post-starburst (PSB) galaxies, identified by strong Balmer absorption and weak nebular emission, provide a key laboratory for studying rapid quenching. Using the final data release…

astro-ph.GA2026

The quenching time and timescale distribution of z~2 quiescent galaxies from precise colour distribution analysis

Vivienne Wild, Ho-Hin Leung, Adam Carnall +1

Understanding when and how galaxies quench their star formation is crucial for understanding the dominant physical processes at play. The spectral energy distribution (SED) of gala…

astro-ph.GA2026

Spatially resolved star-formation histories of local post-starburst galaxies: Starburst and quenching spatial patterns consistent with recent mergers

Ho-Hin Leung, Vivienne Wild, Michail Papathomas +6

Post-starburst (PSB) galaxies, having recently experienced a starburst followed by rapid quenching, are excellent laboratories to probe physical mechanisms that drive starbursts an…

astro-ph.GA2025

The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA

Ho-Hin Leung, Vivienne Wild, Michail Papathomas +2

The quenching of star formation in galaxies is an important aspect of galaxy evolution, but the physical mechanisms that drive it are still not understood. Measuring the spatial di…

astro-ph.GA2025

Low redshift post-starburst galaxies host abundant HI reservoirs

Sara L. Ellison, Qifeng Huang, Dong Yang +8

Studying the gas content of post-starburst (PSB) galaxies can provide valuable clues regarding the process of fast quenching. Although previous works have studied the molecular gas…

astro-ph.GA2025

The infrared luminosity of retired and post-starburst galaxies: A cautionary tale for star formation rate measurements

Vivienne Wild, Natalia Vale Asari, Kate Rowlands +3

In galaxies with significant ongoing star formation there is an impressively tight correlation between total infrared luminosity (L) and H luminosity (L), when…