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A detailed study of feedback from a massive star

Abstract:

We present numerical simulations of a 15 M star in a suite of idealized environments in order to quantify the amount of energy transmitted to the interstellar medium (ISM). We include models of stellar winds, UV photoionization and the subsequent supernova based on theoretical models and observations of stellar evolution. The system is simulated in 3D using RAMSES-RT, an Adaptive Mesh Refinement Radiation Hydrodynamics code. We find that stellar winds have a negligible impact ...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stv251

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
448
Issue:
4
Pages:
3248-3264
Publication date:
2015-03-10
Acceptance date:
2015-02-05
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Source identifiers:
492096
Keywords:
Pubs id:
pubs:492096
UUID:
uuid:cf936ac0-940a-4a95-b652-f7b96323e475
Local pid:
pubs:492096
Deposit date:
2016-07-19

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