output
20162026
most citedMulti-phase Nature of a Radiation-Driven Fountain with Nuclear Starburst in a Low-mass Active Galactic Nucleus

108 citations

9 papers

astro-ph.GA2026

A differentiable hydrodynamical approach to the Milky Way bar pattern speed with CO longitude--velocity data

Junichi Baba, Kohei Hattori

We present a differentiable hydrodynamical framework for modeling barred gas flow in the Milky Way and constraining broad low-loss regions in bar-pattern-speed parameter space from…

astro-ph.GA2026

Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way

Tomoki Yamaguchi, Junichi Baba

We quantify systematic biases in rotation curves inferred from steady, axisymmetric Jeans modelling when the underlying stellar velocity field is non-axisymmetric. Using a high-res…

astro-ph.GA2026

Bar-Informed Kinematic-Distance Mapping of Molecular Gas in the Inner Milky Way

Junichi Baba

We present a bar-informed kinematic-distance (BIKD) method to reconstruct face-on molecular-gas maps of the inner Milky Way from PPV data, relaxing the standard assumption of axisy…

astro-ph.GA2026

Kinematic-Distance Biases in the Inner Milky Way from a Stellar-Dynamically Constrained Bar

Junichi Baba

We quantify how bar-driven non-circular motions bias Milky-Way gas maps inferred with the kinematic-distance (KD) method. KD reconstructions of H\,\textsc{i} and CO surveys assume…

astro-ph.GA2025

Bar-driven Streaming Motions Mimic a Massive Bulge in the Inner Milky Way

Junichi Baba

The circular speed curve of the Milky Way provides a key constraint on its mass distribution, reflecting the axisymmetric component of the gravitational potential. This is especial…

astro-ph.GA2025

Influence of Bar Formation on Star Formation Segregation and Stellar Migration: Implications for Variations in the Age Distribution of Milky Way Disk Stars

Junichi Baba

We present a chemo-dynamical -body/hydrodynamic simulation of an isolated Milky Way-like galaxy to investigate how bar formation influences star formation rates, stellar migrati…