Physics
Scientific paper
Feb 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..736y&link_type=abstract
COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.
Physics
1
Magnetic And Electric Fields, Polarization Of Starlight, Interstellar Medium And Nebulae In External Galaxies, X-Ray
Scientific paper
We analyze the infrared (IR) echelle spectra of 14 T Tauri stars in the Orion Nebular Cluster (ONC) and measure their mean surface magnetic fields by modeling the Zeeman broadening in three magnetically sensitive Ti I lines near 2.2 μm. We combine these measurements with previous measurements of stars in Taurus and the TW Hydrae Association (TWA) to suggest that the strong magnetic fields commonly detected on T Tauri stars could be of a primordial origin. The dominance of strong magnetic pressure over gas pressure in the stellar photospheres might also partially prohibit the production of X-ray emission.
Johns-Krull Christopher M.
Yang Hao
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