astrophysical wopa astrophysical
The workhorse instruments of the current 8-10m class observatories are multi-object spectrographs (MOS), providing comprehensive follow-up of ground-based and space-borne imaging data. With the advent of even deeper imaging surveys from, e.g., HST, VISTA, JWST and Euclid, many science cases require complementary spectroscopy with high sensitivity and good spatial resolution to identify the objects and to measure their astrophysical parameters. The light-gathering power of the 39m E-ELT and its spatial resolution, combined with a MOS, will enable the large samples necessary to tackle some of the key scientific drivers of the E-ELT project, ranging from studies of stellar populations out to the highest-redshift galaxies. Consequently, a MOS-facility is foreseen within the E-ELT instrumentation plan.
Plasma recombination lasers in rapidly cooled stellar atmospheres. astrophysical observations and laboratory results confirm collisional radiative simulation predictions. Quasars are stars in our galaxy.
GEO600 is a gravitational wave detector – a laser interferometer with 600 meter long arms Gravitational waves are tiny ripples in space time caused by astrophysical events e g supernovae or coalescing binaries neutron stars black holes Albert Einstein predicted gravitational waves in 1916 but they have not yet been directly observed
inaf catania astrophysical observatory official home page, il sito fornisce informazioni sulla ricerca presso l'osservatorio astrofisico di catania, su divulgazione dell'astronomia, sulle risorse per la ricerca astrofisica
Covering all aspects of plasma physics including Magnetic and Inertial confinement fusion astrophysical and Space Plasmas Low Density and TechnologicalIndustrial Plasmas Low Temperature Plasmas High Energy Density and Laser Plasmas Dusty and Complex plasmas Plasma Surface interactions Plasma Applications including Medical applications and Plasma Diagnostics
Résultats fournis par Wopa!