collaborators

6 papers

astro-ph.GA2026

From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system

Jihye Hwang, Doris Arzoumanian, Yoshito Shimajiri +5

Hub-filament systems (HFSs) play an important role in the formation of massive stars and star clusters. Although the velocity structures along dense filaments have been studied, th…

astro-ph.GA2026

An Origin of Radially Aligned Filaments in Hub-Filament Systems

Shingo Nozaki, Shu-ichiro Inutsuka

Recent observations have identified hub-filament systems (HFSs) as the primary formation sites of massive stars and star clusters. Some HFSs are characterized by multiple filaments…

astro-ph.GA2025

Self-supervised Synthetic Pretraining for Inference of Stellar Mass Embedded in Dense Gas

Keiya Hirashima, Shingo Nozaki, Naoto Harada

Stellar mass is a fundamental quantity that determines the properties and evolution of stars. However, estimating stellar masses in star-forming regions is challenging because youn…

astro-ph.GA2025

How External Medium outside Prestellar Cores Affects Protostellar Growth: Variations in Accretion Rate and Evolution of Disks and Outflows

Shingo Nozaki, Masahiro N. Machida

We investigate how the external medium surrounding prestellar cores affects the star formation process by conducting three-dimensional resistive magnetohydrodynamic simulations. Th…

astro-ph.GA2025

Extended and Compact Ortho-HD Structures Close to the Moment of Star-Formation: Evidence from ALMA-ACA Observations in Taurus

Kazuki Tokuda, Kenji Furuya, Naofumi Fukaya +8

Observing and characterizing pre- and protostellar cores in the earliest and densest stages of star formation is challenging due to their short timescales and high densities, limit…

astro-ph.GA2025

Tracking Star-Forming Cores as Mass Reservoirs in Clustered and Isolated Regions Using Numerical Passive Tracer Particles

Shingo Nozaki, Hajime Fukushima, Kazuki Tokuda +1

Understanding the physical properties of star-forming cores as mass reservoirs for protostars, and the impact of turbulence, is crucial in star formation studies. We implemented pa…