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...
Đã lưu trong:
| Tác giả chính: | |
|---|---|
| Tác giả khác: | , , , , |
| Định dạng: | article |
| Ngôn ngữ: | Tiếng Anh |
| Được phát hành: |
2024
|
| Những chủ đề: | |
| Truy cập trực tuyến: | https://hdl.handle.net/20.500.12008/48846 |
| Các nhãn: |
Không có thẻ, Là người đầu tiên thẻ bản ghi này!
|
Những quyển sách tương tự: 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
- Final targeting strategy for the sloan digital sky survey IV Apache Point Observatory galactic evolution experiment 2 North Survey
- RR Lyrae stars trace the Milky Way warp
- 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