Physical properties of B-type asteroids from WISE data
Aims: Our aim is to obtain more information about the physical nature of B-type asteroids and extend previous work by studying their physical properties as...
Physical properties of five near-Earth asteroids within the NEOROCKS project
We present photometric data of five near-Earth asteroids (NEAs) obtained in the framework of the NEO Rapid Observation, Characterization, and Key Simulations...
Physical Properties of Lyα Emitters at z ~ 0.3 from UV-to-FIR Measurements
The analysis of the physical properties of low-redshift Lyα emitters (LAEs) can provide clues in the study of their high-redshift analogs. At z ~ 0.3, LAEs are...
Physical properties of NEOs derived from their phase curves
The observation of Near Earth objects (NEOs) allows us to study the physical properties of the smallest size bodies of our Solar System and help impose...
Physical properties of PHA 2014 JO25 from a worldwide observational campaign
The study of minor planets is motivated both by fundamental science of Solar system origins (some of these bodies contain the most pristine materials from the...
Physical properties of simulated galaxy populations at z = 2 - I. Effect of metal-line cooling and feedback from star formation and AGN
We use hydrodynamical simulations from the OverWhelmingly Large Simulations (OWLS) project to investigate the dependence of the physical properties of galaxy...
Physical properties of simulated galaxy populations at z = 2 - II. Effects of cosmology, reionization and ISM physics
We use hydrodynamical simulations from the OverWhelmingly Large Simulations project to investigate the dependence of the physical properties of galaxy...
Physical Properties of Spicules from Simultaneous Spectropolarimetric Observations of He I and Ca II Lines
We present full Stokes observations from SPINOR (Spectro-Polarimeter for INfrared and Optical Regions, at the Dunn Solar Telescope) in the Ca II infrared...
Physical properties of superbubbles in the Antennae galaxies
Mass outflow generated by the dynamical feedback from massive stars is currently a topic of great interest. Using a purpose-developed analysis technique, and...