Authors:
Kuhn, JR
MacQueen, RM
Streete, J
Tansey, G
Mann, I
Hillebrand, P
Coulter, R
Lin, H
Edmunds, D
Judge, P
Citation: Jr. Kuhn et al., Probable detection of a bright infrared coronal emission line of Si ix near 3.93 microns, ASTROPHYS J, 521(1), 1999, pp. 478-482