Tag Archives: Feedback

02 Dec 2014

  • (abs, pdf) Adams et al., AGC198606: A gas-bearing dark matter minihalo?
  • (abs, pdf) Geen et al., A Detailed Study of Feedback from a Massive Star
  • (abs, pdf) Bleuler et al., PHEW: a parallel segmentation algorithm for three-dimensional AMR datasets – application to structure detection in self-gravitating flows
  • (abs, pdf) Grazian et al., The galaxy stellar mass function at 3.5 < z < 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields

08 Oct 2014

  • (abs, pdf) Puchwein et al., The photoheating of the intergalactic medium in synthesis models of the UV background
  • (abs, pdf) Kawamata et al., The sizes of $z\sim6-8$ lensed galaxies from the Hubble Frontier Fields Abell 2744 data
  • (abs, pdf) Kim & Ostriker, Momentum Injection by Supernovae in the Interstellar Medium
  • (abs, pdf) Reed et al., The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies
  • (abs, pdf) Camps & Baes, SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture

17 Sept 2014

  • (abs, pdf) Gallerani et al., First CO(17-16) emission line detected in a z > 6 quasar
  • (abs, pdf) Marassi et al., The origin of the most iron-poor star
  • (abs, pdf) Martizzi et al., Supernova Feedback in an Inhomogeneous Interstellar Medium
  • (abs, pdf) Emonts et al., Outflow of hot and cold molecular gas from the obscured secondary nucleus of NGC3256: closing in on feedback physics
  • (abs, pdf) Smith et al., The Lyman-α signature of the first galaxies
  • (abs, pdf) Richards et al., The SAMI Galaxy Survey: The discovery of a luminous, low-metallicity H II complex in the dwarf galaxy GAMA J141103.98-003242.3

02 Jun 2014

  • (abs, pdf) Cautun et al., Milky Way mass constraints from the Galactic satellite gap
  • (abs, pdf) Cautun et al., Subhalo statistics of galactic halos: beyond the resolution limit
  • (abs, pdf) Hennebelle & Iffrig, Simulations of magnetized multiphase galactic disk regulated by supernovae explosions
  • (abs, pdf) Roos et al., Thermal and radiative AGN feedback have a limited impact on star formation in high-redshift galaxies