stellar astronomy

NESSY · NEw Science from the phase space of old stellar SYstems

SNBinaries · Close binary progenitors and ejected donor remnants of supernovae type Ia

DEFT · Dark energy, non-linearites and effective theories

StarlightWinds · Mass loss in the lives and deaths of massive stars

SF-magnetic-stars · The impact of superfluidity and superconductivity on the magneto-thermal evolution and X-ray observations of neutron stars.

ResolvedJetsHIC · Probing the Strongly-Coupled Quark-Gluon Plasma with Jets

SKPLUS · Super-Kamiokande plus

4 partners · 3 countries

GALFORM_SELFIDM · The impact of collisional dark matter in galaxy formation: Time for a paradigm shift?

LDSNPS · Linking the diversity of Type Ia supernovae to their progenitor systems

MULTIFAST · Variability in Relativistic Jets: the Fastest Time Scales at all Wavelengths

NSMAG · Magnetic Fields in Neutron Stars via Numerical Simulations

AMSP X-RAY BURSTS · Localization of thermonuclear burning on accreting millisecond X-ray pulsars

HER-SFR · Star, gas and dust in star forming regions: studying Star Formation Rate tracers at small galactic scales""

SNIAPROG · A Close Look at Type Ia Supernova Progenitors

DARK-GRB-SN · Optical Studies of Type Ia and Type Ic Supenovae

PROMOPS · Probing models of pulsars through multi wavelength observations

SIMPLE-FEEDBACK · Fedback in low mass galaxies at z>1 : a SIMPLE study

PULSARS WITH LOFAR · Radio pulsars with LOFAR: a study of extreme physics laboratories

ISP · The International Supernova Program (ISP)

HIRVACH · Modelling high resolution spectra of galaxies with variable chemical abundances ratios

GAMMA-RAY BURSTS · Probing star formation throughout the Universe with Gamma-Ray Bursts

GRB-VREESWIJK · Gamma-Ray Burst afterglows: illuminating the early Universe

PADISCLUSDPA · The photometric evolution and age determinations of unresolved star clusters: the effect of selective mass loss from dissolving clusters

RSSGWA · Realistic supercomputer simulations for gravitational wave asteroseismology