SHOCK-cloud interaction and particle acceleration in the southwestern limb of sn 1006
The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relatively tenuous and uniform environment despite interacting with an atomic cloud in its northwestern limb. The X-ray image of SN 1006 reveals an indentation in the southwestern part of the shock front and...
Guardado en:
Autores principales: | Miceli, M., Acero, F., Dubner, G., Decourchelle, A., Orlando, S., Bocchino, F. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_20418205_v782_n2_p_Miceli |
Aporte de: |
Ejemplares similares
-
SHOCK-cloud interaction and particle acceleration in the southwestern limb of sn 1006
Publicado: (2014) -
Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission
por: Miceli, M., et al. -
Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission
Publicado: (2016) -
On the radio polarization signature of efficient and inefficient particle acceleration in supernova remnant SN 1006
por: Reynoso, Estela Marta
Publicado: (2013) -
On the radio polarization signature of efficient and inefficient particle acceleration in supernova remnant SN 1006
por: Reynoso, E.M., et al.