Recovery from Giant Eruptions in Massive Stars

A. Kashi, K. Davidson, R. M. Humphreys

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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.

Original languageEnglish (US)
Title of host publicationThe Physics of Evolved Stars
Subtitle of host publicationA Conference Dedicated to the Memory of Olivier Chesneau
EditorsF. Millour, T. Lanz, E. Lagadec
PublisherEDP Sciences
Pages275-277
Number of pages3
ISBN (Electronic)9782759819072
DOIs
StatePublished - Dec 1 2015
EventPhysics of Evolved Stars Conference 2015 - Nice, France
Duration: Jun 8 2015Jun 12 2015

Publication series

NameEAS Publications Series
Volume71-72
ISSN (Print)1633-4760
ISSN (Electronic)1638-1963

Other

OtherPhysics of Evolved Stars Conference 2015
CountryFrance
CityNice
Period6/8/156/12/15

Bibliographical note

Publisher Copyright:
© 2015 EAS, EDP Sciences.

Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.

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