Kathryn Johnston
Kathryn Johnston Kathryn Johnston
Abundance Patterns in Satellites vs Venn et al (2004) Halo The challenge for Lambda CDM: satellites look chemically different from the halo.... (e.g. Unnavane, Wyse & Gilmore, 1996)
Abundance Patterns in Satellites vs Halo You cannot get .... from.... ...*!@!!!!
- Page 1 and 2: Stellar Halos and Satellite Systems
- Page 3 and 4: Dark matter modeled via merger tree
- Page 5 and 6: Model for Formation of a Halo Color
- Page 7 and 8: Features brighter than 30 mag/ arcs
- Page 9: Model for Formation of a Halo - Hal
- Page 13 and 14: Abundance Patterns in Satellites vs
- Page 15 and 16: Abundance Patterns in Satellites vs
- Page 17 and 18: ... only stars with [alpha/ Fe]
Abundance Patterns in Satellites vs<br />
Venn et al (2004)<br />
Halo<br />
The challenge for<br />
Lambda CDM:<br />
satellites look<br />
chemically different<br />
from the halo....<br />
(e.g. Unnavane,<br />
Wyse & Gilmore,<br />
1996)
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