activity
20242026
collaborators

6 papers

astro-ph.GA2026

Comparison of Bar Formation Mechanisms. IIIA. The role of classical bulges in spontaneous bar formation

Yirui Zheng, Juntai Shen, Bin-Hui Chen

We run a suite of -body simulations to investigate how classical bulges affect bar formation and properties under the internal formation mechanism. We incorporate bulges of vary…

astro-ph.GA2026

Galactic Stellar Halo Luminosity Function

Sarah A. Bird, Chris Flynn, Rudra Sekhri +5

We measure the luminosity function (LF) of the Milky Way's stellar halo, using a magnitude complete, distance limited sample of stars from DR3. Stars with high transverse ve…

astro-ph.GA2026

Bar Formation During a Gaia-Sausage-Enceladus-like Merger Event

Bin-Hui Chen, Juntai Shen, Paola Di Matteo

Bars are among the most prominent galactic structures, yet their formation mechanisms remain incompletely understood. They can form either internally, via dynamical instabilities,…

astro-ph.GA2025

Dependency of the Bar Formation Timescale On The Halo Spin

Bin-Hui Chen, Sandeep Kumar Kataria, Juntai Shen +1

Bars are among the most prominent structures in disk galaxies. While the widely accepted swing-amplification theory provides a qualitative framework for their formation, the detail…

astro-ph.GA2024

Orbital Support and Evolution of CX/OX Structures in Boxy/Peanut Bars

Behzad Tahmasebzadeh, Shashank Dattathri, Monica Valluri +7

Barred galaxies exhibit boxy/peanut or X-shapes (BP/X) protruding from their disks in edge-on views. Two types of BP/X morphologies exist depending on whether the X-wings meet at t…

astro-ph.GA2024

Importance of Initial Condition on Bar Secular Evolution: Role of Halo Angular Momentum Distribution Discontinuity

Sandeep Kumar Kataria, Juntai Shen

The dark matter halo properties, for example, mass, spin and concentration play a significant role in the formation and evolution of bars in disk galaxies. This study highlights th…