16 citations · 85 across the 12 of their papers we have counts for
14 papers
The efficient star-forming regions of stripped-envelope supernovae
M. Solar, M. J. Michałowski, J. Nadolny +13
Massive stars () play a key role in shaping the interstellar medium of galaxies through stellar feedback. However, how these stars form and evolve before explod…
The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae
M. Solar, M. J. Michałowski, J. Nadolny +11
Context. Study of cold molecular hydrogen gas (hereafter molecular gas) provides crucial insights into its interplay with star-forming regions. However, the connection between mole…
Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c
Bruno Šlaus, Natalia Gotkiewicz, Michał J. Michałowski +6
Understanding which stars explode as which type of supernovae (SNe) is crucial to measure their contribution to the metal production and feedback halting star formation. Most of th…
Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
M. P. Koprowski, J. V. Wijesekera, J. S. Dunlop +5
We present a new determination of the evolving far-infrared galaxy luminosity function (FIR LF) and the resulting inferred evolution of dust-obscured star-formation rate density (S…
Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems
Bastian Ayala, Joseph P. Anderson, G. Pignata +8
Type IIb supernovae (SNe IIb) often exhibit an early light curve excess (EE) preceding the main peak powered by radioactive nickel decay. The physical origin of this early emission…
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…
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…
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…
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…
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…
The Fate of the Interstellar Medium in Early-type Galaxies. II. Observational Evidence for Morphological Quenching
Aleksandra Leśniewska, Michał Jerzy Michałowski, Christa Gall +4
The mechanism by which galaxies stop forming stars and get rid of their interstellar medium (ISM) remains elusive. Here, we study a sample of more than two thousand elliptical gala…
Main Sequence to Starburst Transitioning Galaxies: Gamma-ray Burst Hosts at
Jakub Nadolny, Michał Jerzy Michałowski, J. Ricardo Rizzo +8
Star-forming galaxies populate a main sequence (MS), a well-defined relation between stellar mass (M*) and star-formation rate (SFR). Starburst (SB) galaxies lie significantly abov…
Automatic algorithm to obtain values via Fourier Transform in BeSOS database
Martín Solar, Catalina Arcos, Michel Curé +2
Be stars are found to rotate close to their critical rotation and therefore they are considered as an important laboratory of study for stellar rotation. In this context, we obtain…
Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations
Martin Solar, . Patricia B. Tissera, Jose A. Hernandez-Jimenez
The exploration of the spatial distribution of chemical abundances in star-forming regions in galactic discs provides clues to understand the complex interplay of physical processe…