output
20062026
most citedCurrent Star Formation in the Ophiuchus and Perseus Molecular Clouds: Constraints and Comparisons from Unbiased Submillimeter and Mid-Infrared Surveys. II

141 citations

20 papers

astro-ph.GA2026

Radar-Chart Analysis of Star-Formation Quenching Stages Across Circular Velocity Curve Classes in Nearby CALIFA Galaxies

Veselina Kalinova, Dario Colombo

We analyze the circular velocity curves of 215 non-active galaxies from the Calar Alto Legacy Integral Field spectroscopy Area survey. Using radar-chart analysis, we compare two cl…

astro-ph.GA2026

Variability of Sagittarius A* at 3 GHz on minute-scale with MeerKAT

K. Kaur, I. Rammala-Zitha, A. Basu +21

The supermassive black hole Sagittarius A* (Sgr A*) exhibits temporal and spectral variability across the electromagnetic spectrum. However, variability at radio frequencies below…

astro-ph.SR2026★ 5 cited

The drastic impact of Eddington-limit induced mass ejections on massive star populations

D. Pauli, N. Langer, A. Schootemeijer +6

Massive stars are the key engines of the Universe. However, their evolution and thus their ionizing feedback are still not fully understood. One of the largest gaps in current stel…

astro-ph.SR2025★ 7 cited

A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars

Harim Jin, Norbert Langer, Andrea Ercolino +1

Massive stars often evolve in binary systems, in which binary interactions significantly affect their evolution. Massive stars in the Galaxy serve as valuable testbeds for this due…

astro-ph.HE2025★ 1 cited

A broadband study of FRB20240114A with the Effelsberg 100-m radio telescope

P. Limaye, L. G. Spitler, N. Manaswini +5

We present Effelsberg 100-m telescope observations of the hyperactive repeating fast radio burst source FRB 20240110A, discovered by CHIME/FRB in January 2024. Using the Ultra Broa…

astro-ph.SR2025★ 4 cited

The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction

Andrea Ercolino, Harim Jin, Norbert Langer +3

The observational properties of core-collapse supernovae (CC-SNe) are shaped by the envelopes of their progenitors. In massive binary systems, mass-transfer alters the pre-SN struc…