Measuring magnetic fields near and far with the SKA via the zeeman effect
Paper in proceeding, 2014

The measurement of Zeeman splitting in spectral lines-both in emission and absorption-can provide direct estimates of the magnetic field strength and direction in atomic and molecular clouds, both in our own MilkyWay and in external galaxies. This method will probe the magnetic field in the warm and cold neutral components of the interstellar medium, providing a complement to the extensive SKA Faraday studies planning to probe the field in the ionized components.

Author

T. Robishaw

National Research Council Canada

J. A. Green

SKA Organisation

G. Surcis

Joint Institute for VLBI in Europe (JIVE)

Wouter Vlemmings

Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics

Other publications Research

A. M. S. Richards

Jodrell Bank Centre for Astrophysics

S. Etoka

University of Hamburg

T. L. Bourke

SKA Organisation

V. Fish

Massachusetts Institute of Technology (MIT)

M. D. Gray

Jodrell Bank Centre for Astrophysics

H. Imai

Kagoshima University

B. Kramer

Max Planck Society

J. McBride

University of California

E. Momjian

National Radio Astronomy Observatory

A. Sarma

DePaul University

A. Zijlstra

Jodrell Bank Centre for Astrophysics

Proceedings of Science

18248039 (eISSN)

Vol. 9-13-June-2014

Subject Categories (SSIF 2011)

Astronomy, Astrophysics and Cosmology

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7/12/2024

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