Suzaku Observations of Galaxy Groups (and related systems)
Suzaku Observations of Galaxy Groups (and related systems) Suzaku Observations of Galaxy Groups (and related systems)
XMM-Newton and Chandra • To higher redshift, more detail, and larger radius GEMS --Chandra (Rasmussen and Ponman 2007) scaled temperature Si/Fe (grsa) r/r 500
XMM-Newton and Chandra • High resolution spectra, multi-phase models NGC 5044 Si/Fe profile Tamura et al. 2003 Buote et al. 2003
- 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: XMM-Newton and Chandra More heating
- 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 and 24: Abundance Profiles courtesy K. Mats
- Page 25 and 26: Abundance Patterns Similar pattern
- Page 27 and 28: Abundances in Groups with Suzaku: :
- Page 29: Abundances in Groups with Suzaku: :
XMM-Newton <strong>and</strong> Ch<strong>and</strong>ra<br />
• To higher redshift, more detail, <strong>and</strong> larger radius<br />
GEMS --Ch<strong>and</strong>ra (Rasmussen <strong>and</strong> Ponman 2007)<br />
scaled temperature<br />
Si/Fe (grsa)<br />
r/r 500
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