Observing Magnetic Fields in Star-Forming Regions

Details Observing Magnetic Fields in Star-Forming Regions Observing Magnetic Fields in Star-Forming Regions

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.295...27c&link_type=abstract

Astrophysics and Space Science, Volume 295, Issue 1-2, pp. 27-36

Astronomy and Astrophysics

Astrophysics

1

Magnetic Fields, Star-Forming Regions, Zeeman Effect, Masers, Polarization

Scientific paper

Magnetic field strengths and directions can be estimated using many different observational techniques that span a wide range of wavelengths. Each observational method favours different regimes of scale size, density and other physical conditions. The available techniques and their ranges of applicability are briefly described and the current status of observations is reviewed, with particular emphasis on high-resolution observations of star-forming regions.

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