XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)
Aims: We report the first detailed X-ray study of the supernova remnant (SNR) G304.6+0.1, achieved with the XMM-Newton mission. Methods: The powerful imaging capability of XMM-Newton was used to study the X-ray characteristics of the remnant at different energy ranges. The X-ray morphology and spect...
Guardado en:
| Autores principales: | Combi, Jorge Ariel, Albacete Colombo, Juan Facundo, Sánchez Ayaso, E., Romero, Gustavo Esteban, Martí, J., Luque Escamilla, P. L., Muñoz Arjonilla, A. J., Sánchez Sutil, J. R., López Santiago, J. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2010
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/82532 |
| Aporte de: |
Ejemplares similares
-
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)
por: Combi, Jorge A., et al.
Publicado: (2010) -
Discovery of thermal X-ray emission in the supernova remnant G337.8-0.1 (Kes 41)
por: Combi, Jorge Ariel, et al.
Publicado: (2008) -
Molecular environments of the supernova remnant G359.1-0.5
por: Eppens, Laura Karina, et al.
Publicado: (2020) -
Observaciones del remanente de supernova G296.5+10.0 con el satélite XMM-Newton
por: Eppens, Laura Karina, et al.
Publicado: (2022) -
Detailed study of SNR G306.3 - 0.9 using XMM-Newton and Chandra observations
por: Combi, J.A., et al.