A BeppoSAX observation of the cooling flow cluster Abell 2029
| dc.creator | Molendi, Silvano | |
| dc.creator | De Grandi, Sabrina | |
| dc.date | 1999-10-15 | |
| dc.date.accessioned | 2026-07-07T02:33:52Z | |
| dc.date.available | 2026-07-07T02:33:52Z | |
| dc.description | We present results from a BeppoSAX observation of the cooling flow cluster Abell 2029. The broad band spectrum (2-35 keV) of the cluster, when fitted with a model including a cooling flow component and a one temperature thermal component, yields a temperature of 8.3+/-0.2 keV and a metal abundance of 0.46+/-0.03 in solar units, for the latter. No evidence of a hard X-ray excess is found in the PDS spectrum. By performing a spatially resolved spectral analysis we find that the projected temperature and abundance drop with increasing radius, going from about 8 keV and 0.5 (solar units) at the cluster core to about 5 keV and 0.2 (solar units) at about 1.2 Mpc. | |
| dc.description | To appear in Astronomy & Astrophysics Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9910284 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9910284 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15020 | |
| dc.subject | Astrophysics | |
| dc.title | A BeppoSAX observation of the cooling flow cluster Abell 2029 | |
| dc.type | text |