Three-dimensional adaptive mesh refinement hydrodynamical simulations of the wind–wind
collision between the enigmatic supermassive star η Car and its mysterious companion star …

In order to study the distribution of gas and ionizing radiation around η Car and their
implications for its likely companion star, we have examined high-excitation emission lines …

We reconstruct the evolution of η Car in the last two centuries under the assumption that the
two 19th century eruptions were triggered by periastron passages and through this …

We report near-infrared spectroscopic observations of the Eta Carinae massive binary
system during 2008–2009 using the CRIRES spectrograph mounted on the 8 m UT 1 Very …

Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …

We report on Hα spectroscopy of the 2009.0 spectroscopic event of η Carinae collected via
SMARTS observations using the Cerro Tololo Interamerican Observatory 1.5 m telescope …

In late 2006, ground-based photometry of η Car plus the Homunculus showed an
unexpected decrease in its integrated apparent brightness, an apparent reversal of its long …

The first chapter introduces Eta Carinae, highlighting why it is so interesting and worth
studying, while Chapter 2 reviews the theory of radiation-driven winds from hot, massive (> …

ABSTRACT Three dimensional (3D) adaptive-mesh refinement (AMR) hydrodynamical
simulations of the windwind collision between the enigmatic super-massive star η Car and …

Three dimensional (3D) adaptive-mesh refinement (AMR) hydrodynamical simulations of the
wind-wind collision between the enigmatic super-massive star\etacar and its mysterious …