@inproceedings{aadde6fdbb1844a38e95cc5ebfadd61f,
title = "Recovery from Giant Eruptions in Massive Stars",
abstract = "We perform radiation hydrodynamic simulations to study how very massive stars recover from giant eruptions. The post eruption star experience strong mass loss due to strong winds, driven by radial pulsations in the star's interior, that operate by the κ-mechanism. The mass loss history obtained in our simulations resembles η Car's history.",
author = "A. Kashi and K. Davidson and Humphreys, {R. M.}",
note = "Publisher Copyright: {\textcopyright} 2015 EAS, EDP Sciences.; Physics of Evolved Stars Conference 2015 ; Conference date: 08-06-2015 Through 12-06-2015",
year = "2015",
month = dec,
day = "1",
doi = "10.1051/eas/1571061",
language = "אנגלית",
series = "EAS Publications Series",
publisher = "EDP Sciences",
pages = "275--277",
editor = "F. Millour and T. Lanz and E. Lagadec",
booktitle = "The Physics of Evolved Stars",
address = "צרפת",
}