Polarization observations reveal dominant toroidal magnetic fields of a few milligauss in a protostellar outflow, sufficient to collimate it and supporting magneto-centrifugal launching.
A., Asgari-Targhi, M
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Analytical expressions for ALP-photon conversion in transient compact stars yield an updated bound g_aγ < 5×10^{-12} GeV^{-1} for m_a ≲ 10^{-9} eV from SN 1987A, plus sensitivity forecasts for future Galactic SN and NSM observations.
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Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow
Polarization observations reveal dominant toroidal magnetic fields of a few milligauss in a protostellar outflow, sufficient to collimate it and supporting magneto-centrifugal launching.
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Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
Analytical expressions for ALP-photon conversion in transient compact stars yield an updated bound g_aγ < 5×10^{-12} GeV^{-1} for m_a ≲ 10^{-9} eV from SN 1987A, plus sensitivity forecasts for future Galactic SN and NSM observations.