The Magellanic Clouds are surrounded by an extended network of gaseous structures. Chief
among these is the Magellanic Stream, an interwoven tail of filaments trailing the Clouds in …

The disks of disk galaxies contain a substantial fraction of their baryonic matter and angular
momentum, and much of the evolutionary activity in these galaxies, such as the formation of …

Positional, structural, and dynamical parameters for all dwarf galaxies in and around the
Local Group are presented, and various aspects of our observational understanding of this …

The Close Binary Fraction of Solar-type Stars Is Strongly Anticorrelated with Metallicity -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

We present the first ever global, spatially resolved reconstruction of the star formation history
(SFH) of the Large Magellanic Cloud (LMC), based on the application of our StarFISH …

We present uniformly measured star formation histories (SFHs) of 60 nearby (D≲ 4 Mpc)
dwarf galaxies based on color–magnitude diagrams of resolved stellar populations from …

We present the first detailed assessment of the large-scale rotation of any galaxy based on
full three-dimensional velocity measurements. We do this for the LMC by combining our …

Context. The new VISual and Infrared Telescope for Astronomy (VISTA) has started
operations. Over its first five years it will be collecting data for six public surveys, one of …

We present a novel pair of numerical models of the interaction history between the Large
and Small Magellanic Clouds (LMC and SMC, respectively) and our Milky Way (MW) in light …

We use recently derived ages for 61 Milky Way (MW) globular clusters (GCs) to show that
their age–metallicity relation (AMR) can be divided into two distinct, parallel sequences at …