Context. Recent observational findings have suggested a positive correlation between the
occurrence rates of inner super-Earths and outer giant planets. These results raise the …

We introduce a new model for the accretion and feedback of supermassive black hole
(SMBH) binaries to the ketju code, which enables us to resolve the evolution of SMBH …

We present measurements of the galaxy luminosity and stellar mass function in a 3.71 deg 2
(0.3 Mpc 2) area in the core of the Virgo Cluster, based on ${u}^{\ast} $ griz data from the …

We present a uniform analysis of the stellar initial mass function (IMF) from integrated light
spectroscopy of 15 compact stellar systems (11 globular clusters in M31 and 4 ultra compact …

A gap in exoplanets' radius distribution has been widely attributed to the photoevaporation
threshold of their progenitors' gaseous envelope. Giant impacts can also lead to substantial …

In recent years, a growing zoo of compact stellar systems (CSSs) have been found whose
physical properties (mass, size, velocity dispersion) place them between classical globular …

Globular clusters (GCs) are evolved stellar systems containing entire populations of
millisecond pulsars (MSPs), which are efficient γ-ray emitters. Observations of this emission …

It has been suggested that ultracompact dwarf (UCD) galaxies are the 'threshed'remains of
larger galaxies. Simulations have revealed that extensive tidal-stripping may pare a galaxy …

We use the hydrodynamical EAGLE simulation to predict the numbers, masses, and radial
distributions of tidally stripped galaxy nuclei in massive galaxy clusters, and compare these …

We use the hydrodynamical EAGLE simulation to test if ultracompact dwarf galaxies (UCDs)
can form by tidal stripping by predicting the ages and metallicities of tidally stripped galaxy …