Weak emission lines and chemical composition in ionized nebula
The analysis of emission line spectra of photoionized nebulae allows us to determine the chemical composition of the interstellar medium from the solar...
Weave: Cluster Surveys: A New Vision of the role of the environment in Galazy Evolution
The environment plays a key role in the formation and evolution of galaxies. Clusters of galaxies are the most massive and virialized structures known in the...
WEAVE: Exploring new scientific horizons through spectroscopic surveys.
The William Herschel Telescope (WHT) has been a key player in the take-off of Spanish astronomy in the last 25 years. With the access of the Spanish community...
WEAVE: Exploring the Cosmic Original Symphony, from Stars to galaxy clusters
WEAVE-ECOS is an unoriented research project that integrates two senior researchers and their team in order to efficiently exploit the first science data from...
WEAVE: the next-generation wide-field spectrograph for the William Herschel Telescope
The world-class 4.2m William Herschel telescope (WHT), with its comprehensive instrument suite at the superb site of the Observatorio del Roque de los Muchachos...
X-ray binaries: accretion, ejection and dynamical masses
Black-holes and neutron stars are extremely important astrophysical objects, which become unique laboratories of extreme physics when found within X-ray...
X-ray binaries: accretion, ejection and dynamical masses
Black-holes and neutron stars are extremely important astrophysical objects, which become unique laboratories of extreme physics when found within X-ray...
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only...