most citedThe fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation

14 citations · 21 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA20242 cited

Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since

Jakub Nadolny, Michał J. Michałowski, Massimiliano Parente +4

Recent high-redshift () spatially resolved observations with the James Webb Space Telesescope have shown the evolution of the star formation rate (SFR) surface density ($Σ_{\r…

astro-ph.GA2024

The Fate of the Interstellar Medium in Early-type Galaxies. V. AGN Feedback from Optical Spectral Classification

Oleh Ryzhov, Michał J. Michałowski, J. Nadolny +6

Quenching of star-formation plays a fundamental role in galaxy evolution. This process occurs due to the removal of the cold interstellar medium (ISM) or stabilization against coll…

astro-ph.GA20245 cited

The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies

Jakub Nadolny, Michał J. Michałowski, Massimiliano Parente +6

Removing cold interstellar medium (ISM) from a galaxy is central to quenching star formation. However, the exact mechanism of this process remains unclear. The objective of this wo…

astro-ph.GA202414 cited

The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation

Michał J. Michałowski, C. Gall, J. Hjorth +15

Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that…