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20122026
most citedDust Evolution in Galaxy Cluster Simulations

56 citations · 235 across the 28 of their papers we have counts for

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Showing 2026Show all

8 papers · 1 filter

astro-ph.CO2026

The relevance of the cosmic microwave background for cosmology

Pavel Kroupa, Eda Gjergo, Nikolaos Samaras

Within the Hot Big Bang picture, as usually interpreted in the standard LCDM framework and its hierarchical scenario for elliptical galaxy assembly, the cosmic microwave background…

astro-ph.GA2026

The MAGPI Survey: Emission Line Products Data Release and the Role of Spectroscopic Aperture Covering Fraction on the Balmer Decrement-Stellar Mass Relation

A. J. Battisti, E. G. M. Muller, E. Wisnioski +27

The Middle Ages Galaxy Properties with Integral field spectroscopy (MAGPI) survey is a Large Program on the European Southern Observatory Very Large Telescope using the MUSE instru…

astro-ph.GA2026

The MAGPI Survey: Evidence for Non-Universal Resolved Dust Attenuation Relations Beyond the Local Universe

A. Mailvaganam, T. Zafar, P. Corcho-Caballero +39

We study the spatially resolved relation between dust attenuation () and star formation rate surface density () in galaxies from the MAGPI survey ($0.25 < z…

astro-ph.GA2026★ 2 cited

Baryonic mass budgets in the central regions of the Bullet Cluster and their consistency with strong lensing in MOND

Dong Zhang, Hosein Haghi, Elena Asencio +8

Strong lensing observations of the Bullet Cluster have traditionally been regarded as strong evidence for dark matter and a major challenge to Milgromian dynamics (MOND). The offse…

astro-ph.GA2026

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation

Soonchul Choi, Eda Gjergo, Youngman Kim +1

Scandium, titanium, and vanadium can be synthesized primarily in massive stars. Yet many of the current Galactic chemical evolution models under-produce these elements at early epo…

astro-ph.GA2026

Limited imprint of high-mass IMF variations on sodium abundances in main-sequence galaxies

Ziyi Guo, Donatella Romano, Zhiqiang Yan +10

Growing evidence suggests that the stellar initial mass function (IMF) varies systematically across galaxies, deviating from the canonical Milky Way form. Such variations would mod…

astro-ph.GA2026

The mmax-Mecl relation in the LEGUS clusters

Marie Zinnkann, Tereza Jerabkova, Zhiqiang Yan +6

The relation between the maximum stellar mass in a very young cluster (mmax) and the total stellar mass of the cluster (Mecl), known as the mmax-Mecl relation, remains debated in t…

astro-ph.GA2026

The Initial Mass Function as the Equilibrium State of a Variational Process: why the IMF cannot be sampled stochastically

Eda Gjergo, Zhiyu Zhang, Pavel Kroupa

The stellar initial mass function (sIMF) is often treated as a stochastic probability distribution, yet such an interpretation implies Poisson noise that is inconsistent with growi…