most citedTracking Protostellar Variability in Massive Protoclusters with ALMA: I. Insights from QUARKS and MaMMOtH

1 citations

6 papers

cond-mat.supr-con2026

Superconductivity on the verge of metal-insulator transition in CuZnIrS probed by SR

K. M. Kojima, M. Miyazaki, M. Hiraishi +6

The thiospinel CuIrS undergoes a metal-insulator transition below 230 K, which is suppressed by substitution of Cu with Zn (CuZnIrS) to induce…

astro-ph.HE2026

Electron-capture Supernova Candidates from Light Curves: Implications for Their Progenitors and Explosion Properties

Masato Sato, Nozomu Tominaga, Sergei I. Blinnikov +5

Core-collapse supernovae are explosions of massive stars. While most massive stars end as iron-core-collapse supernovae, less massive stars are expected to explode as electron-capt…

astro-ph.EP2026

Rapid and Predictive Planet Population Synthesis Model (RAPPS) I. Upgraded model and resulting synthetic populations

Tadahiro Kimura, Masahiro Ikoma

Exoplanet surveys have revealed a wide diversity of planetary systems, requiring integrated models of planet formation to explain their origin. Planet population synthesis (PPS) mo…

hep-ph2026

Delineating neutral and charged mesons in magnetic fields

Toru Kojo, Sakura Itatani

We investigate the properties of neutral and charged mesons in magnetic fields, from weak-field to strong-field regimes. To develop analytic insights, we employ a non-relativistic…

astro-ph.GA20261 cited

Tracking Protostellar Variability in Massive Protoclusters with ALMA: I. Insights from QUARKS and MaMMOtH

Yuhan Yang, Tie Liu, Sheng-Yuan Liu +22

Millimeter/submillimeter variability is often attributed to dynamical disk-mediated accretion, yet detection is limited to low-mass protostars in nearby clouds. Recent observations…

astro-ph.HE2026

The broad-lined type Ic supernova 2020lao experienced an energetic explosion with no central-engine signatures

M. D. Stritzinger, T. J. Moriya, S. Bose +18

We present infant-phase observations of the SN Ic-BL 2020lao, including optical spectroscopy beginning 48 hrs after explosion. The explosion time was constrained by power-law fits…