Abstract
Recent efforts to account for the observed LX - TX relation of galaxy clusters has led to suggestions that the ICM has an apparent "entropy oor" at the level of K0 ≳ 300 keV cm2. Here, we propose new tests based on the thermal SZ effect and on the Mgas - TX trend (from X-ray data) to probe the level of the excess entropy in the ICM. We show that these new tests lend further support to the case for a high entropy oor in massive clusters.
Original language | English (US) |
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Pages (from-to) | 315-316 |
Number of pages | 2 |
Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volume | 17 |
State | Published - 2003 |
Externally published | Yes |
Event | Galaxy Evolution: Theory and Observations - Cozumel, Mexico Duration: Apr 8 2002 → Apr 12 2002 |
Keywords
- Cosmology: theory
- Galaxies: clusters
- X-rays: galaxies
ASJC Scopus subject areas
- Space and Planetary Science
- Astronomy and Astrophysics