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Probable detection of a bright infrared coronal emission line of Si IX near 3.93 microns

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Mann,  I.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Mann, I., Kuhn, J. R., MacQueen, R. M., Streete, J., Tansey, G., Hillebrand, P., et al. (1999). Probable detection of a bright infrared coronal emission line of Si IX near 3.93 microns. Astrophysical Journal, 521, 478-482.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-DEA5-4
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