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: 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: 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...
Dentro de las acciones de divulgación del proyecto Interreg EELabs, la madrugada del 4 de enero, el canal sky-live.tv retransmitirá la máxima actividad de la...
“Las mujeres somos parte de CTA; gran parte de su ciencia se hace gracias a nosotras”
CTA es un proyecto internacional con más de 1400 miembros de más de 200 instituciones de 31 países. Es, por ello, una infraestructura de una gran diversidad que...