Suzaku Observations of Galaxy Groups (and related systems)
Suzaku Observations of Galaxy Groups (and related systems) Suzaku Observations of Galaxy Groups (and related systems)
from heasarc.gsfc.nasa.gov
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19.11.2014
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Abundance Profiles courtesy K. Sato
Abundance Patterns Similar pattern within systems, and from system to system -- Fe/α≥1 Matsushita et al. 2007 courtesy Y. Fukazawa
- Page 1 and 2: Suzaku Observations of Galaxy Group
- Page 3 and 4: Matter in the Universe (the modern
- Page 5 and 6: Sub-types of interest X-ray: NASA/C
- Page 7 and 8: Why Study Groups in X-rays? • The
- Page 9 and 10: ROSAT and ASCA Highlights • Abund
- Page 11 and 12: XMM-Newton and Chandra More heating
- Page 13 and 14: XMM-Newton and Chandra • High res
- Page 15 and 16: Cool (
- Page 17 and 18: Temperature Structure XIS requires
- Page 19 and 20: Abundances RGS: N(?), O, Ne, Mg, Fe
- Page 21 and 22: Complementarity, , e.g. NGC 4472
- Page 23: Abundance Profiles courtesy K. Mats
- Page 27 and 28: Abundances in Groups with Suzaku: :
- Page 29: Abundances in Groups with Suzaku: :
Abundance Patterns<br />
Similar pattern within<br />
<strong>systems</strong>, <strong>and</strong> from system<br />
to system -- Fe/α≥1<br />
Matsushita et al. 2007<br />
courtesy Y. Fukazawa
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