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Clump formation through colliding stellar winds in the Galactic Centre

Published online by Cambridge University Press:  09 February 2017

D. Calderón Open the ORCID record for D. Calderón [Opens in a new window] ,
J. Cuadra ,
A. Ballone ,
M. Schartmann ,
A. Burkert ,
J. Prieto  and
S. Gillessen
D. Calderón*
Affiliation:
Instituto de Astrofísica, Pontificia Universidad Católica de Chile
J. Cuadra
Affiliation:
Instituto de Astrofísica, Pontificia Universidad Católica de Chile
A. Ballone
Affiliation:
Max-Planck-Institute for Extraterrestrial Physics, Germany Universitätssternwarte der Ludwig-Maximilians-Universität, Germany
M. Schartmann
Affiliation:
Center for Astrophysics and Supercomputing, Swinburne University of Technology, Australia
A. Burkert
Affiliation:
Max-Planck-Institute for Extraterrestrial Physics, Germany Universitätssternwarte der Ludwig-Maximilians-Universität, Germany
J. Prieto
Affiliation:
Departamento de Astronomía, Universidad de Chile
S. Gillessen
Affiliation:
Max-Planck-Institute for Extraterrestrial Physics, Germany
*
*email: [email protected]
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Abstract

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We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW.

Keywords

hydrodynamics – instabilities – stars: windsoutflows – Galaxy: centre
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S322: The Multi-Messenger Astrophysics of the Galactic Centre , July 2016 , pp. 204 - 205
Copyright
Copyright © International Astronomical Union 2017 

References

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