The Herschel view of the nebula around the luminous blue variable star AG Carinae

TL;DR

This study uses Herschel infrared observations to analyze the nebula around LBV star AG Car, revealing its structure, dust composition, and mass, and providing insights into the star's evolutionary history.

Contribution

It presents detailed infrared imaging and spectroscopic analysis of AG Car's nebula, including dust modeling and mass estimates, offering new constraints on the star's mass-loss history and evolutionary phase.

Findings

Nebula appears as a clumpy ring extending up to 1.2 pc.

Dust mass estimated at approximately 0.2 solar masses.

Ejection likely occurred during a cool LBV phase for a ~55 solar mass star.

Abstract

Far-infrared Herschel PACS imaging and spectroscopic observations of the nebula around the luminous blue variable (LBV) star AG Car have been obtained along with optical imaging in the Halpha+[NII] filter. In the infrared light, the nebula appears as a clumpy ring shell that extends up to 1.2 pc with an inner radius of 0.4 pc. It coincides with the Halpha nebula, but extends further out. Dust modeling of the nebula was performed and indicates the presence of large grains. The dust mass is estimated to be ~ 0.2 Msun. The infrared spectrum of the nebula consists of forbidden emission lines over a dust continuum. Apart from ionized gas, these lines also indicate the existence of neutral gas in a photodissociation region that surrounds the ionized region. The abundance ratios point towards enrichment by processed material. The total mass of the nebula ejected from the central star amounts to ~ 15 Msun, assuming a dust-to-gas ratio typical of LBVs. The abundances and the mass-loss rate were used to constrain the evolutionary path of the central star and the epoch at which the nebula was ejected, with the help of available evolutionary models. This suggests an ejection during a cool LBV phase for a star of ~ 55 Msun with little rotation.