Distribution of the high-velocity clouds in the Galactic halo
Context. There is a connection between the kinematics and sky distribution of the high velocity clouds (HVCs) and the spatial velocity and orbital plane of the Magellanic Clouds (MCs) that allow us to conclude that most HVCs were ejected from the Clouds, some hundreds of Myrs ago, probably by an enc...
Guardado en:
| Autor principal: | Olano, Carlos Alberto |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2008
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84248 |
| Aporte de: |
Ejemplares similares
-
The high-velocity clouds and the Magellanic Clouds
por: Olano, Carlos Alberto
Publicado: (2004) -
A new survey for high velocity HI detections in the Southern Hemisphere
por: Morras, Ricardo, et al.
Publicado: (2000) -
Age-metallicity relation in the Magellanic Clouds clusters
por: Livanou, E., et al.
Publicado: (2013) -
The VISCACHA survey: how star clusters tell the Magellanic Clouds’ history
por: Dias, B., et al.
Publicado: (2022) -
A view of Large Magellanic Cloud HII regions N159, N132, and N166 through the 345-GHz window
por: Paron, S., et al.