In force date
Call year
2015
Investigator
Manuel Linares Alegret
Financial institution
Financing program
Financing subprogram
Amount granted to the IAC Consortium
18.849,00 €
Related projects
![The illustration is inspired in the system V404 Cygni, and represents both the companion star and the accretion disc surrounding the black hole, as well as ejection processes in the form of a jet and wind. Black hole in outburst](/sites/default/files/styles/crop_square_2_2_to_320px/public/images/project/%C3%87Imagen%20TMD.jpg?h=25367c22&itok=0HYcf1S9)
Black holes, neutron stars, white dwarfs and their local environment
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only confirmation of the existence of stellar mass black holes via dynamical mass measurements, but also the best opportunity for probing high-gravity environments and the physics of accretion; the most
Montserrat
Armas Padilla