Abstract The “Homunculus” nebula around Eta Carinae is one of our most valuable tools for
understanding the extreme nature of episodic pre-supernova mass loss in the most massive …

I review recent observational results concerning the structure, kinematics, mass, and dust
properties of the Homunculus nebula around η Carinae. The review is biased toward …

The discovery of the Little Homunculus in η Carinae has at least two implications:(1) the mini
eruption of 1890 may indeed have produced bipolar ejecta;(2) the formation process of the …

The remarkable, interrelated stellar and nebular constituents of η Carinae's habitat, the giant
Carina Nebula (NGC 3372), are reviewed. They are relevant to the interpretation of η Car …

Eta Carinae provides a unique example to investigate a massive star in a late evolutionary
phase and how CNO-processed material is ejected and mixed with the interstellar medium …

The nature and origin of the molecular gas component located in the circumstellar vicinity of
η Carinae are still far from being completely understood. Here, we present Atacama Large …

The first paper in this series took a direct census of energy input from the known OB stars in
the Carina Nebula, and in this paper we study the global properties of the surrounding …

We present follow-up optical imaging and spectroscopy of one of the light echoes of η
Carinae's nineteenth century Great Eruption discovered by Rest et al. By obtaining images …

Eta Carinae is a massive evolved star that is undergoing prodigious and highly convulsive
mass loss. The Eta Carinae Treasury Team (PT. Kris Davidson) recently conducted an …

We have constructed an interacting winds scenario to account for the geometric and
kinematic properties of the Homunculus in η Carinae as seen in recent Hubble Space …