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...
Saved in:
| Main Author: | |
|---|---|
| Other Authors: | , , , , |
| Format: | article |
| Language: | English |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://hdl.handle.net/20.500.12381/3665 https://doi.org/10.1093/mnras/stae308 |
| Tags: |
No Tags, Be the first to tag this record!
|
Similar Items: Structure, kinematics, and time evolution of the Galactic warp from Classical Cepheids
- Structure, kinematics, and time evolution of the Galactic warp from Classical Cepheids
- Estudio de ondulaciones en el disco de la Vía Láctea con estrellas pulsantes
- RR Lyrae stars trace the Milky Way warp
- Final targeting strategy for the sloan digital sky survey IV Apache Point Observatory galactic evolution experiment 2 North Survey
- The outer disc in shambles: Blind detection of Monoceros and the ACS with Gaia’s astrometric sample
- Validation of the Bond et al. (2010) SDSS-derived kinematic models for the Milky Way’s disk and halo stars with Gaia Data Release 3 proper motion and radial velocity data