Numerical simulations of the 1840s great eruption of $\eta$ Carinae: I. Revisiting the explosion scenario

Abstract

In this work, we present new two-dimensional hydrodynamical simulations of the major eruption of $\eta$ Car in the 1840s, which resulted in the formation of a bipolar nebula that is commonly known as the large Homunculus. In our numerical models, we have included the high-speed component of 10000 km s${}^{-1}$, detected in recent observations, that provides direct evidence of an explosive event. Here, we investigate whether such a violent explosion is able to explain both the shape and the dynamical evolution of $\eta$ Car's nebula. As in our previous work, we have assumed a two-stage scenario for $\eta$ Car's eruption: a slow outflow phase during a few decades before the eruption followed by the explosive event. From the collision of these outflow phases, the large Homunculus is produced. Our numerical simulations show that such scenario does not resemble some of the observed physical features and the expansion of the nebula. Notwithstanding, we also explore other injection parameters (mass-loss rate and ejection velocity) for these outflow phases. In particular, we find that an explosion with an intermediate-speed of 1000 km s${}^{-1}$ is able to reproduce the morphology and the kinematical age of the large Homunculus.

Accepted to A&A

References in corpus (3)

• Pulsational Pair-Instability Supernovae
• Possible Implications of Mass Accretion in Eta Carinae
• $\eta$ Carinae Baby Homunculus Uncovered by ALMA

Cited by in corpus (1)

• The bright, dusty aftermath of giant eruptions & H-rich supernovae. Late interaction of supernova shocks & dusty circumstellar shells