C-19 and Hot, Wide Star Streams
The C-19 star stream has the abundance characteristics of an unusually metal-poor globular cluster but kinematically is uncharacteristically hot and wide for a cluster stream, having a line-of-sight velocity dispersion of 7 ± 2 km s ^−1 and a 1 σ width of 240 pc. We show that the tidal dissolution...
Gardado en:
| Principais autores: | , , , , , , , |
|---|---|
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Assuntos: | |
| Acceso en liña: | https://doi.org/10.3847/1538-4357/ade4ce |
| Tags: |
Sen Etiquetas, Sexa o primeiro en etiquetar este rexistro!
|