Da. Allen et Dj. Hillier, THE SHAPE OF THE HOMUNCULUS NEBULA AROUND ETA-CARINAE, Proceedings - Astronomical Society of Australia, 10(4), 1993, pp. 338-341
From extensive spectroscopic observations we derive the three-dimensio
nal structure of the Homunculus Nebula surrounding eta Carinae. The an
alysis shows that the two lobes are hollow and incomplete, and that th
e gas was ejected at similar epoch. Consequently the distribution of m
aterial we see reflects its initial velocity. Using the observed expan
sion velocity, and the known time of ejection, we derive a distance to
eta Car of 2.2 +/- 0.2 kpc.