Structure, kinematics, and time evolution of the Galactic warp from Classical Cepheids

The warp is a well-known undulation of the Milky Way disc. Its structure has been widely studied, but only since Gaia DR2 has it been possible to reveal its kinematic signature beyond the solar neighbourhood. In this work, we present an analysis of the warp traced by Classical Cepheids by means of a...

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Bibliographic Details

Main Author:	Cabrera Gadea, Mauro Ramón (author)
Other Authors:	Mateu, Cecilia (author), Ramos, Pau (author), Romero-Gómez, Mercé (author), Antoja, T. (author), Aguilar, Luis (author)
Format:	article
Language:	English
Published:	2024
Subjects:	Stars variables Galaxy disc Galaxy evolution Galaxy kinematics and dynamics Galaxy structure Cepheids
Online Access:	https://hdl.handle.net/20.500.12008/48846
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