output
20062026
most citedHyperon mixing and universal many-body repulsion in neutron stars

169 citations

27 papers

cs.RO2026

Few-Shot Adaptation to Non-Stationary Environments via Latent Trend Embedding for Robotics

Yasuyuki Fujii, Emika Kameda, Hiroki Fukada +3

Robotic systems operating in real-world environments often suffer from concept shift, where the input-output relationship changes due to latent environmental factors that are not d…

astro-ph.HE2026★ 1 cited

Transverse Oscillations and Wave Propagation in the Magnetically Dominated M87 Jet

Hyunwook Ro, Motoki Kino, Kazuhiro Hada +6

We present an in-depth analysis of transverse oscillations in the M87 jet, as identified in our previous study (Ro et al. 2023a), which reported oscillatory patterns with a charact…

astro-ph.HE2026★ 1 cited

Locating the missing large-scale emission in the jet of M87* with short EHT baselines

Boris Georgiev, Paul Tiede, Sebastiano D. von Fellenberg +280

In Very-Long Baseline Interferometric arrays, nearly co-located stations probe the largest scales and typically cannot resolve the observed source. In the absence of large-scale st…

astro-ph.HE2025★ 4 cited

Probing jet base emission of M87* with the 2021 Event Horizon Telescope observations

Saurabh, Hendrik Müller, Sebastiano D. von Fellenberg +282

We investigate the presence and spatial characteristics of the jet base emission in M87* at 230 GHz, enabled by the enhanced uv coverage in the 2021 Event Horizon Telescope (EHT) o…

astro-ph.HE2025★ 20 cited

Horizon-scale variability of M87* from 2017--2021 EHT observations

The Event Horizon Telescope Collaboration

We report three epochs of polarized images of M87* at 230\,GHz using data from the Event Horizon Telescope (EHT) taken in 2017, 2018, and 2021. The baseline coverage of the 2021 ob…

astro-ph.EP2024★ 5 cited

Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks . Time-dependent model

Ayumu Kuwahara, Michiel Lambrechts, Hiroyuki Kurokawa +2

The observed dust rings and gaps in protoplanetary disks could be imprints of forming planets. Even low-mass planets in the one-to-ten Earth-mass regime, that do not yet carve deep…