Chandra Analysis of Abell 496
| dc.creator | Dupke, Renato A. | |
| dc.creator | White III, Raymond E. | |
| dc.date | 2001-10-02 | |
| dc.date.accessioned | 2026-07-07T02:00:35Z | |
| dc.date.available | 2026-07-07T02:00:35Z | |
| dc.description | We present preliminary results of imaging and spectral analysis of the cluster A496 with the S3 chip on-board the Chandra satellite. We confirm the presence of a cooling flow and radial gradients in elemental abundances. The cluster's core has clear signs of substructures (sharp edges, cavities), similar to those recently found in other cooling flow clusters. The O/Fe ratio distribution indicates that the gas in the core of the cluster is significantly enriched by SN Ia ejecta. | |
| dc.description | 4 LaTeX pages (newpasp.sty) with six embedded EPS figures; to appear in "The X-ray Universe at Sharp Focus", eds. S. Vrtilek, E. Schlegel and L. Kuhi, ASP Conference Series References | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0110070 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0110070 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3459 | |
| dc.subject | Astrophysics | |
| dc.title | Chandra Analysis of Abell 496 | |
| dc.type | text |