Results 131 to 140 of about 123,440 (246)
Accretion in supergiant High Mass X-ray Binaries
EPJ Web of Conferences, 2014 Supergiant High Mass X-ray Binary systems (sgHMXBs) consist of a massive, late type, star and a neutron star. The massive stars exhibits strong, radiatively driven, stellar winds.
Manousakis Antonios +2 more
doaj +1 more source
Nuclear astrophysics in our time: supernovae, neutron stars and binary neutron star mergers. [PDF]
Eur Phys J Spec Top, 2021 Bandyopadhyay D.
europepmc +1 more source
Equation of State of Neutron Star Matter and Neutron Star Models [PDF]
, 1971 Satoru Ikeuchi +3 more
openalex +1 more source
An Emission Line in the Hard X-Ray Spectrum of Hercules X-1: Quantized Cyclotron Emission from the Neutron Star [PDF]
, 1977 W. Pietsch +5 more
openalex +1 more source
Physics Letters BParity-violating electron scattering experiments on Ca48 (CREX) and Pb208 (PREX-2) offer valuable insight into the isovector properties of finite nuclei, providing constraints for the density dependence of the nuclear equation of state, which is crucial ...
P.S. Koliogiannis, E. Yüksel, N. Paar
doaj +1 more source
Black hole-neutron star coalescence: Effects of the neutron star spin on jet launching and dynamical ejecta mass. [PDF]
Phys Rev D, 2020 Ruiz M +3 more
europepmc +1 more source