RR Lyrae stars trace the Milky Way warp
Context. The outskirts of the Milky Way disc have been known to be warped since the late 1950s. Although various stellar populations have shown an underlying warped distribution, the relation between the age of the population and the warp they trace remains an open question. Understanding this relat...
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| Beste egile batzuk: | , |
| Formatua: | article |
| Hizkuntza: | ingelesa |
| Argitaratua: |
2024
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| Gaiak: | |
| Sarrera elektronikoa: | https://hdl.handle.net/20.500.12381/3669 |
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Antzeko izenburuak: RR Lyrae stars trace the Milky Way warp
- Estudio de ondulaciones en el disco de la Vía Láctea con estrellas pulsantes
- Structure, kinematics, and time evolution of the Galactic warp from Classical Cepheids
- Structure, kinematics, and time evolution of the Galactic warp from Classical Cepheids
- Empirical completeness assessment of the Gaia DR2, Pan-STARRS 1, and ASAS-SN-II RR Lyrae catalogues
- Systematic census of RR Lyrae in Milky Way stellar streams
- 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