The dark energy plus cold dark matter (ΛCDM) cosmological model has been a
demonstrably successful framework for predicting and explaining the large-scale structure of …

The distribution of the non-luminous matter in galaxies of different luminosity and Hubble
type is much more than a proof of the existence of dark particles governing the structures of …

We present new H i interferometric observations of the gas-rich ultra-diffuse galaxy AGC
114905, which previous work, based on low-resolution data, identified as an outlier of the …

We report the discovery of 47 low surface brightness objects in deep images of a 3× 3 field
centered on the Coma cluster, obtained with the Dragonfly Telephoto Array. The objects …

Recently a population of large, very low surface brightness, spheroidal galaxies was
identified in the Coma cluster. The apparent survival of these ultra-diffuse galaxies (UDGs) …

We develop analytic methods for studying the formation of galaxies by gas condensation
within massive dark halos. Our scheme applies to cosmogonies where structure grows …

THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE
SURVEY - IOPscience Skip to content IOP Science home Accessibility Help Search Journals …

Recent observations have revealed the existence of an abundant population of faint, low
surface brightness (SB) galaxies, which appear to be numerous and ubiquitous in nearby …

We present a sample of 115 very low optical surface brightness, highly extended, H i-rich
galaxies carefully selected from the ALFALFA survey that have similar optical absolute …

We present a detailed prescription for the modelling of galaxy formation in hierarchical
theories of structure formation. Our model incorporates the formation and merging of dark …