Due to their low surface brightness, dwarf galaxies are particularly susceptible to tidal forces.
The expected degree of disturbance depends on the assumed gravity law and whether they …

Using the latest cosmological hydrodynamic N-body simulations of groups and clusters, we
study how location in phase-space coordinates at z= 0 can provide information on …

The structure of a dwarf galaxy is an important probe of the effects of stellar feedback and
environment. Using an unprecedented sample of 223 low-mass satellites from the ongoing …

Context. Studies of low surface brightness (LSB) galaxies in nearby clusters have revealed a
sub-population of extremely diffuse galaxies with central surface brightness of μ 0, g′> 24 …

The Next Generation Virgo Cluster Survey. XXIII. Fundamentals of Nuclear Star Clusters over
Seven Decades in Galaxy Mass - IOPscience This site uses cookies. By continuing to use this …

We present the properties of the globular clusters (GCs) and nuclear star clusters (NSCs) of
low-mass (10 5.5< M⋆< 10 8.5 M⊙) early-type satellites of Milky Way–like and small group …

Taking advantage of the Sloan Digital Sky Survey Stripe82 data, we have explored the
spatial distribution of ultra-diffuse galaxies (UDGs) within an area of 8× 8 Mpc2 centred …

We present an analysis of archival HST/ACS imaging in the F475W (g 475), F606W (V 606),
and F814W (I 814) bands of the globular cluster (GC) system of a large (3.4 kpc effective …

Ultra-diffuse galaxies (UDGs) have the sizes of giants but the luminosities of dwarfs. A key to
understanding their origins comes from their total masses, but their low surface brightnesses …

Using a case example, the authors explore how the counseling field's participation in the
discourse of heterosexist dominance fosters microaggressions toward sexual and gender …