activity
20192026
most citedAzimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations

16 citations · 85 across the 12 of their papers we have counts for

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Showing 2024Show all

5 papers · 1 filter

astro-ph.GA2024★ 2 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.SR2024★ 14 cited

Binary progenitor systems for Type Ic supernovae

Martín Solar, Michał J. Michałowski, Jakub Nadolny +18

Core-collapse supernovae are explosions of massive stars at the end of their evolution. They are responsible for metal production and for halting star formation, having a significa…

astro-ph.GA2024★ 5 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.GA2024★ 14 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…