X-ray Emission and Incidence of Magnetic Fields in Massive Stars of the Orion Nebula Cluster

Details X-ray Emission and Incidence of Magnetic Fields in Massive Stars of the Orion Nebula Cluster X-ray Emission and Incidence of Magnetic Fields in Massive Stars of the Orion Nebula Cluster

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..405..547p&link_type=abstract

Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, proceedings of the conference held 17-21 Septembe

Astronomy and Astrophysics

Astronomy

Scientific paper

Magnetic fields have been frequently invoked as a likely source of
variability and confinement of the winds of the Orion Nebula Cluster
massive stars. We carried out sensitive ESPaDOnS observations to search
for direct evidence of such fields, detecting unambiguous Zeeman
signatures in three objects.

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