Magnetic Milky Way

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Proceedings titleEAS Publications Series
ConferenceThe Role of the Disk-Halo Interaction in Galaxy Evolution: Outflows vs. Infall?, 18 August 2008 through 22 August 2008, Espinho
Pages8186; # of pages: 6
SubjectMagnetic field line; Milky ways; Spiral arms; Publishing; Galaxies
AbstractSpiral 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). © EAS, EDP Sciences 2012.
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AffiliationNational Research Council Canada (NRC-CNRC); NRC Herzberg Institute of Astrophysics (HIA-IHA)
Peer reviewedYes
NPARC number21269216
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Record identifier017d7a25-aff1-440f-8c78-5d739bb3d061
Record created2013-12-12
Record modified2016-05-09
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