Gas Transfer between the Inner 3 kpc Disk and the Galactic Central Molecular Zone

Gas Transfer between the Inner 3 kpc Disk and the Galactic Central Molecular Zone

We uncovered a more tilted molecular gas structure with highly negative velocities located near the dust lane. Our observations show that the approaching gas flows from the overshoot process are captured by the gravitational potential of the bar and then flow toward the Galactic central molecular zo...

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Bibliographic Details
Main Authors: Yang Su, Shiyu Zhang, Yan Sun, Ji Yang, Fujun Du, Min Fang, Qing-Zeng Yan, Shaobo Zhang, Zhiwei Chen, Xuepeng Chen, Xin Zhou, Lixia Yuan, Yuehui Ma
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Interstellar medium
Molecular clouds
Galaxy kinematics
Milky Way Galaxy
Galaxy structure
Milky Way dynamics
Online Access:https://doi.org/10.3847/1538-4357/adc38e
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