Heat conduction in X-ray clusters: Spitzer over 3
| dc.creator | Gruzinov, Andrei | |
| dc.date | 2002-03-04 | |
| dc.date.accessioned | 2026-07-07T02:02:59Z | |
| dc.date.available | 2026-07-07T02:02:59Z | |
| dc.description | Effective heat conduction in a random variable magnetic field should be equal to one third of the Spitzer's value. Recent observations indicate that this heat conduction is sufficient to account for the bremsstrahlung in cooling X-ray clusters. | |
| dc.description | 3 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0203031 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0203031 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4237 | |
| dc.subject | Astrophysics | |
| dc.title | Heat conduction in X-ray clusters: Spitzer over 3 | |
| dc.type | text |