Observations of galaxies with future X-ray observatories
| dc.creator | Fabbiano, G. | |
| dc.date | 2001-06-22 | |
| dc.date.accessioned | 2026-07-25T18:11:47Z | |
| dc.description | Normal galaxies are faint and complex X-ray sources that provide very powerful probes for fundamental astrophysical questions. Examples include: the study of populations of X-ray emitting sources; the study of the entire spectrum of black-hole phenomena; and galaxy formation and evolution in interaction with the surrounding environment. While exciting, all these fields {\bf require} Chandra sub-arcsecond resolution, and at least comparable spectral capabilities. They also require much large collecting areas. I argue that this is the direction we must plan for future X-ray observatories. | |
| dc.description | conference proceeding; New Century of X-Ray Astronomy Yokohama Symposia, Yokohama, Japan 6-8 March 2001 http://www.astro.isas.ac.jp/conference/newcentx/ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0106414 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0106414 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/54139 | |
| dc.subject | Astrophysics | |
| dc.title | Observations of galaxies with future X-ray observatories | |
| dc.type | text |