Financing subprogram: SUBPROGRAMA ESTATAL DE GENERACIÓN DE CONOCIMIENTO
Grant
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: 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...