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Could magnetic fields produce outwards stellar migration?

Published online by Cambridge University Press:  21 March 2017

Eduardo Battaner
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, Spain Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
Estrella Florido
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, Spain Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
Almudena Zurita
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, Spain Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
Ana Guijarro
Affiliation:
Centro Astronómico Hispano Alemán, Calar Alto, (CSIC-MPG)
Tomás Ruiz-Lara
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, Spain Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
Isabel Pérez
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, Spain Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
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Extract

We propose a qualitative explanation for the light radial profile of a spiral galaxy based on the quantitative magnetic model of truncations (Battaner et al. 2002) in which when stars are born (hence the magnetic force acting on the progenitor gas cloud is no longer at work) migrate to larger orbits or escape.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

Battaner, E., Florido, E., & Jiménez-Vicente, J. 2002, A&A, 388, 213 Google Scholar
Florido, E., Battaner, E., Zurita, A., & Guijarro, A. 2007, A&A, 472, L39 Google Scholar
Ruiz-Lara, T. 2016, PhD. Univ. Granada Google Scholar
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