Marszewski et al., available on arXiv Abstract: The unprecedented infrared spectroscopic capabilities of JWST have provided high-quality interstellar medium (ISM) metallicity measurements and enabled characterization …
Wijers et al., available on arXiv Abstract: The properties of warm-hot gas around ~L* galaxies can be studied with absorption lines from highly ionized metals. …
Byrne et al., available on arXiv Abstract: Feedback from supermassive black holes is believed to be a critical driver of the observed color bimodality of …
Bassini et al., available on arXiv Abstract: Observations show a tight correlation between the stellar mass of galaxies and their gas-phase metallicity (MZR). This relation …
Porter et al., available on arXiv Abstract: We present an investigation of clustered stellar feedback in the form of superbubbles identified within eleven galaxies from …
Trapp et al., available on arXiv Abstract: Fueling star formation in large, disky galaxies, requires a continuous supply of gas accreting into star-forming regions. Previously, …
Ponnada et al., available on arXiv Abstract: Cosmic rays (CRs) may drive outflows and alter the phase structure of the circumgalactic medium, with potentially important …
Mercedes-Feliz et al., available on arXiv Abstract: We investigate the formation of dense stellar clumps in a suite of high-resolution cosmological zoom-in simulations of a …
Sands et al., available on arXiv Abstract: While galaxy rotation curves provide one of the most powerful methods for measuring dark matter profiles in the …
Choban et al., available on arXiv Abstract: Observations indicate dust populations vary between galaxies and within them, suggesting a complex life cycle and evolutionary history. …