Abstract
We summarize the key observations made in recent observations of X-ray sources in early-type galaxies. Typically about half of the X-ray binaries in early-type galaxies are in globular clusters, they are preferentially found in metal rich globular clusters, and there is no indication that cluster age is an important parameter. Theoretical challenges are presented by these results.
Original language | English |
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Pages (from-to) | 73-74 |
Number of pages | 2 |
Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volume | 20 |
DOIs | |
State | Published - 2004 |
Event | IAU Colloquium 194 - Compact Binaries in the Galaxy and Beyond - La Paz, B.C. Sur, Mexico Duration: Nov 17 2003 → Nov 22 2003 |
Keywords
- Galaxies: Individual (NGC 3115,NGC 4365, NGC 4472)
- Galaxies: Star clusters
- Stars: Mass loss
- X-rays: Binaries