We report high-precision X-ray monitoring observations in the 0.4–10 keV band of the
luminous, long-period colliding wind binary Eta Carinae, up to and through its most recent X …

Abstract The Tarantula Nebula (30 Doradus, 30 Dor) is the most important star-forming
complex in the Local Group, offering a microscope on starburst astrophysics. At its heart lies …

We simulate the hydrodynamics of the wind flow in the B [e] supergiant binary system GG
Carinae and obtain the mass accretion rate on to the secondary and the observed light …

Just recently, we are starting to explore the γ-ray sky at energies above 100TeV. A detailed
understanding of the emission at these extreme energies is therefore of paramount …

Colliding winds of massive stars in binary systems (CWB) have been proposed as potential
sites of relativistic cosmic-ray acceleration and non-thermal very-high-energy (VHE) photons …

Only a few gamma-ray sources have been established as proton accelerators over the last
decades, among them two extraordinary binary systems, the massive colliding wind binary …

The paper considers a solution for recovery of spectral density informativity for a generalized
class of non-integrable signals. The standard Fourier transform, with a limited set of …