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European Astronomical Society Publications Series European Astronomical Society Publications Series

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Magnetic Milky Way

Published online by Cambridge University Press:  17 September 2012

J.P. Vallée
J.P. Vallée
Affiliation:
Herzberg Institute of Astrophysics, National Research Council Canada, 5071 West Saancih Road, Victoria, BC V9E 2E7, Canada
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Abstract

Spiral arm shapes, locations, and velocities can be well determined, when model pitfalls are avoided (Vallée 2008a). Similarly, circularly orbiting gas and magnetic field lines can cross the spiral arms, when observational pitfalls are avoided (Vallée 2008b).

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 56: The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall? , 2012 , pp. 81 - 86
Copyright
© EAS, EDP Sciences, 2012

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References

Brown, J.C., Haverkorn, M., Gaensler, B.M., et al., 2007, ApJ, 663, 258CrossRef
Rand, R.J.& Lyne, R.G., 1994, MNRAS, 268, 497CrossRef
Roberts, W.W.R., 1975, Vistas Astron., 19, 91CrossRef
Vallée, J.P., 1988, AJ, 95, 750CrossRef
Vallée, J.P., 2005, ApJ, 619, 297CrossRef
Vallée, J.P., 2008a, AJ, 135, 1301CrossRef
Vallée, J.P., 2008b, ApJ, 681, 303CrossRef
Vallée, J.P., 2011, New Astron. Rev., 55, 91CrossRef

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