New Worlds, New Horizons with X-ray Astronomy

Saturday, March 8, 2014

The impact of mechanical AGN feedback on the formation of massive early-type galaxies. (arXiv:1403.1257v1 [astro-ph.CO])





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Sunday, March 2, 2014

Evolution of the cosmic web. (arXiv:1401.7866v1 [astro-ph.CO])





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Posted by Randall Smith at 2:48 PM No comments:
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The X-ray Properties of Weak Lensing Selected Galaxy Clusters. (arXiv:1402.4484v1 [astro-ph.CO])





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AGN-driven outflows without quenching in simulations of high-redshift disk galaxies. (arXiv:1402.4482v1 [astro-ph.CO])





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General relativistic modelling of the negative reverberation X-ray time delays in AGN. (arXiv:1402.0899v1 [astro-ph.HE])





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Evolution of perturbations and cosmological constraints in decaying dark matter models with arbitrary decay mass products. (arXiv:1402.2972v1 [astro-ph.CO])





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      • The impact of mechanical AGN feedback on the forma...
      • Evolution of the cosmic web. (arXiv:1401.7866v1 [a...
      • The X-ray Properties of Weak Lensing Selected Gala...
      • AGN-driven outflows without quenching in simulatio...
      • General relativistic modelling of the negative rev...
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About this Blog

'New Worlds, New Horizons' (NWNH) is the title of the 2010 Decadal Survey of Astronomy & Astrophysics report, which pointed out the key role of X-ray astronomy both today and in the future. This blog collects papers relevant to X-ray astronomy and the themes outlined in NWNH.

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Randall Smith
I'm an astrophysicist at the Smithsonian Astrophysical Observatory in Cambridge, MA. Any opinions expressed are my personal views and not those of the Smithsonian.
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NWNH

NWNH
Report of the 2010 Decadal Survey of Astronomy and Astrophysics

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