Context. The distribution of member stars in the surroundings of an open cluster (OC) can shed light on the process of its formation, evolution, and dissolution...
Structure and dynamics of isolated internetwork Ca II H bright points observed by SUNRISE
Aims: We aim to improve our picture of the low chromosphere in the quiet-Sun internetwork by investigating the intensity, horizontal velocity, size and lifetime...
Structure and star formation in disk galaxies. II. Optical imaging
We present optical observations of a sample of 57 spiral galaxies and describe the procedures followed to reduce the data. We have obtained images in the...
Studies of cosmic microwave background structure at Dec.=+40 deg - I. The performance of the Tenerife experiments
The direct identification of structure in the cosmic microwave background (CMB) is a major objective of observational cosmology. We present a detailed...
Context. The results obtained by asteroseismology with data from space missions such as CoRoT and Kepler are providing new insights into stellar evolution...
Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth
We investigate the evolution of supermassive black holes in the `Evolution and Assembly of GaLaxies and their Environments' (EAGLE) cosmological hydrodynamic...
Supersonic Motions in Giant H II Regions: Handling 3D Data with Matador
Bidimensional spectroscopy with good spatial and spectral resolution, sampling a particular emission line over the whole emitting area, is shown here to be the...
Surface composition and dynamical evolution of two retrograde objects in the outer solar system: 2008 YB3 and 2005 VD
Most of the objects in the trans-Neptunian belt (TNb) and related populations move in prograde orbits with low eccentricity and inclination. However, the list...
Surface density profiles of collisionless disc merger remnants
We present a detailed surface density analysis of a large sample of simulated collisionless mergers of disc galaxies with bulges (mass ratios 1:1, 2:1, 3:1, 4:1...