Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1
| dc.creator | Giacani, E. | |
| dc.creator | Loiseau, N. | |
| dc.creator | Dubner, G. | |
| dc.creator | Smith, M. J. S. | |
| dc.date | 2005-11-16 | |
| dc.date.accessioned | 2026-07-07T06:45:10Z | |
| dc.date.available | 2026-07-07T06:45:10Z | |
| dc.description | We report on new VLA radio and XMM-Newton X-ray observations of the SNR G352.7-0.1. These high sensitivity, high resolution data reveal that G352.7-0.1 belongs to the thermal composite morphological class. Small scale structures in radio and X-ray emission are not always correlated and are different for the different X-rays bands examined. The distance to G352.7-0.1 can be constrained between 6.6 and 8.4 kpc. The study of the HI suggests that G352.7-0.1 is located within a cavity probably created by the stellar wind of the precursor star. | |
| dc.description | 2 pages, 2 figures. To appear in the proceedings of "The X-Ray Universe 2005" conference, 2005 Sept 26-30, El Escorial, Madrid, Spain | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0511477 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0511477 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/102980 | |
| dc.subject | Astrophysics | |
| dc.title | Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1 | |
| dc.type | text |