Yearly Archives: 2013
24 Dec 2013
- (abs, pdf) McKinney et al., Three-Dimensional General Relativistic Radiation Magnetohydrodynamical Simulation of Super-Eddington Accretion, using a new code HARMRAD with M1 Closure
- (abs, pdf) Vanzella et al., LBT/MODS1 spectroscopic confirmation of two faint sources at z=6.4 magnified by the CLASH / Frontier Fields cluster MACSJ0717.5+3745: towards the characterization of star-forming galaxies at … Continue Reading ››
20 Dec 2013
- (abs, pdf) Tescari et al., Simulated star formation rate functions at $\bf{z\sim4-7}$, and the role of feedback in high-$\bf{z}$ galaxies
- (abs, pdf) Offner et al., The Origin and Universality of the Stellar Initial Mass Function
- (abs, pdf) Whalen et al., Pair-Instability Supernovae in the Local Universe
- (abs, pdf) Padoan et … Continue Reading ››
19 Dec 2013
18 Dec 2013
17 Dec 2013
- (abs, pdf) Johnson et al., Discovery of a transparent sightline at {\rho} < 20 kpc from an interacting pair of galaxies
- (abs, pdf) Ball, CANFAR+Skytree: A Cloud Computing and Data Mining System for Astronomy
- (abs, pdf) Ball, Focus Demo: CANFAR+Skytree: A Cloud Computing and Data Mining System for Astronomy
16 Dec 2013
13 Dec 2013
- (abs, pdf) Maschberger et al., The relation between accretion rates and the initial mass function in hydrodynamical simulations of star formation
- (abs, pdf) Zhang et al., Radiation Transfer of Models of Massive Star Formation. III. The Evolutionary Sequence
- (abs, pdf) Rémy-Ruyer et al., Gas-to-Dust mass ratios in local galaxies over a … Continue Reading ››
12 Dec 2013
- (abs, pdf) Stacy et al., The Mutual Interaction Between Population III Stars and Self-Annihilating Dark Matter
- (abs, pdf) Cunnama et al., The environmental dependence of neutral hydrogen in the GIMIC simulations
- (abs, pdf) Dobbs et al., Formation of Molecular Clouds and Global Conditions for Star Formation
New paper: On the contribution of active galactic nuclei to reionization
Reionization is an extended process where the whole universe transitions from neutral to ionized between 300 and 1,000 million years after the Big Bang. While it has been established that galaxies are the main drivers of reionization and that active galactic nuclei (AGN) are unimportant during this process, very few have made an effort to … Continue Reading ››