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The circumstellar medium surrounding rotating massive stars asgrb precursors

Published online by Cambridge University Press:  22 July 2013

B. Pérez-Rendón ,
J. Higuera ,
G. García-Segura ,
A. Santillán  and
L. Hernández-Cervantes
B. Pérez-Rendón
Affiliation:
Depto. de Investigación en Física, Universidad de Sonora, Hermosillo, Sonora, México
J. Higuera
Affiliation:
Departamento de Física, Universidad de Sonora, Hermosillo, Sonora, México
G. García-Segura
Affiliation:
Instituto de Astronomía, UNAM, Ensenada, Baja California, México
A. Santillán
Affiliation:
Dirección General de Cómputo y de Tecnologías de Información y Comunicación, DGCTIC, UNAM, México City, México
L. Hernández-Cervantes
Affiliation:
Instituto de Astronomía, UNAM, Ciudad Universitaria, México City, México
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Abstract

Long duration Gamma Ray Bursts (LGRB) are thought to originate from massive rotatingstars and the interaction of their expanding jet will be affected by the structure oftheir circumburst medium. In this work we use rotating stellar models of massive stars todetermine the state of circumbust material in various types of progenitor scenarios and wedescribe how this external matter can appear in GRB observations.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 61: Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe , 2013 , pp. 371 - 373
Copyright
© EAS, EDP Sciences 2013

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References

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