reference_papers


 * 02/08/11**
 * Andrey. During lunch presentations today, I mentioned that observational constraints on the rates of prompt and delayed SNIa indicate that numerically prompt SNIa (t<~1e8 yrs) are swamped compared to delayed SNIa (t>2e8 yrs). For metallicity issue it depends on what one calls prompt and delayed - i.e., at what t yields would be changing considerably. The reason I defined prompt SNe to be t<2e8 yrs is that SNe progenitors of t~2e8 yrs were part of the previous models before evidence for prompt SNe was discovered. So they are not new. The observational study I referred to is this: [|Maoz et al. 2010]
 * Alexey: sedimentation speed: faster for light elements (mainly because Coulomb drag is proportional to Z**2):[| Gilfanov & Sunyaev 1984], [|Chuzhoy & Loeb 2004]**


 * 02/09/11**


 * Andrey. I've mentioned new results on entropy profiles in AMR simulations that are much better agreement with observations (i.e., have monotonically decreasing entropy profiles without large core). The paper in question is[| Dubois et al. 2010] At some point we should have simulation-focused discussion about this issue as there are indications that this result is not unique to AGN feedback but can arise in any scenario where proto-clusters build up steeper pressure gradient in the core.


 * 02/10/11**
 * Fabjan et al. X-ray mass proxies from hydrodynamic simulations of galaxy clusters (paper I): [[file:fabjan.scaling.pdf]]


 * 02/12/11**
 * A. Simionescu et al "Baryons at the Edge of the X-ray Brightest Galaxy Cluster ", Science in press,[|arXiv/1102.2429]
 * O. Urban et al. "X-ray Spectroscopy of the Virgo Cluster out to the Virial Radius", MNRAS in press [| arXiv/1102.2430]


 * 02/14/11**
 * [|More et al. paper] on properties of the FOF halos
 * Paper on correlation between Bondi accretion rate and radio power of central AGN, brought up in cool core group discussion: [|Balmaverde et al. 2008]


 * 02/23/11**
 * Falkovich G, Gawedzki K and Vergassola M (2001) **Particles and fields in fluid turbulence.**[|//Rev. Mod. Phys.// **73** : 913--75] [[|PDF]]


 * 02/25/11**
 * [|Special issue of Advances in Astronomy on non-Gaussianity]. The issue was edited by Dragan Huterer, Eiichiro Komatsu, and Sarah Shandera and includes 15 (mostly review) articles on cosmological predictions and observational signatures of non-Gaussian features in the primordial fluctuation spectrum.


 * 02/28/11**
 * Allen, Evrard and Mantz, **Cosmological Parameters from Observations of Galaxy Clusters** [|ARAA (in prep)] [[|PDF] (2.0 MB)] 58 page review paper aimed at young scientists entering the field. Contains roughly 300 references. We anticipate a 2011 publication date.
 * Leitner, S. & Kravtsov, A., //"Fuel Efficient Galaxies: Sustaining Star Formation with Stellar Mass Loss"//, 2011, ApJ submitted [[|arXiv/1011.1252]] - paper brought up during Cool Core discussion.