Tracing the Galactic Disk with the Kinematics of Gaia Cepheids

Tracing the Galactic Disk with the Kinematics of Gaia Cepheids

Classical Cepheids (CCs) are excellent tracers for understanding the structure of the Milky Way disk. The latest Gaia Data Release 3 provides a large number of line-of-sight velocity information for Galactic CCs, offering an opportunity for studying the kinematics of the Milky Way. We determine the...

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Bibliographic Details
Main Authors: Xiaoyue Zhou, Xiaodian Chen, Licai Deng, Shu Wang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy structure
Milky Way disk
Stellar kinematics
Galaxy rotation curves
Cepheid variable stars
Online Access:https://doi.org/10.3847/1538-4357/ad2c08

Internet

https://doi.org/10.3847/1538-4357/ad2c08

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