Tag Archives: GC

30 Jul 2012

(abs, pdf) Blom et al., The SLUGGS Survey: Globular cluster system kinematics and substructure in NGC 4365
(abs, pdf) Tremblin et al., 3D simulations of globules and pillars formation around HII regions: turbulence and shock curvature
(abs, pdf) Ferrara, First Stars IV: Summary Talk
(abs, pdf) Viel et al., The impact of feedback from galaxy formation on the Lyman-alpha transmitted flux

(abs, pdf) Larsen et al., Constraints on mass loss and self-enrichment scenarios for the globular clusters of the Fornax dSph

(abs, pdf) Elmegreen et al., Formation of Metal-Poor Globular Clusters in Lyman alpha Emitting Galaxies in the Early Universe
(abs, pdf) Yozin & Bekki, The Fornax dwarf galaxy as a remnant of recent dwarf-dwarf merging in the Local Group

(abs, pdf) Clementini et al., Variability and star formation in Leo T, the lowest luminosity star-forming galaxy known today
(abs, pdf) Peñarrubia et al., The coupling between the core/cusp and missing satellite problems
(abs, pdf) Schaerer et al., Properties of z~3-6 Lyman break galaxies. II. Testing star formation histories and the SFR-mass relation with ALMA and near-IR spectroscopy
(abs, pdf) Gerke et al., Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
(abs, pdf) Maxwell et al., Building the Stellar Halo Through Feedback in Dwarf Galaxies
(abs, pdf) Brooks & Zolotov, Why Baryons Matter: The Kinematics of Dwarf Spheroidal Satellites
(abs, pdf) Umbreit & Rasio, Constraining Intermediate-Mass Black Holes in Globular Clusters
(abs, pdf) Schnittman et al., X-ray Spectra from MHD Simulations of Accreting Black Holes
(abs, pdf) Capuzzo-Dolcetta et al., A fully parallel, high precision, N-body code running on hybrid computing platforms

(abs, pdf) Marks et al., Evidence for top-heavy stellar initial mass functions with increasing density and decreasing metallicity
(abs, pdf) Dayal et al., The physics of the fundamental metallicity relation
(abs, pdf) Schaerer, Evolutionary synthesis models as a tool and guide towards the first galaxies