Abstract
We discuss joint observations of flares on the dMe star AD Leo made with IUE, the VLA, and the Tinsley photometer at the University of Hawaii's 24-inch reflector on Mauna Kea. We find that optical emission is correlated with C IV while radio emission is better correlated with He II. We reach some tentative conclusions concerning timescales and source characteristics.
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© 1987 Springer-Verlag
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Gary, D.E., Byrne, P.B., Butler, C.J. (1987). IUE/OPTICAL/VLA flares on AD Leo. In: Linsky, J.L., Stencel, R.E. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 291. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-18653-0_117
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DOI: https://doi.org/10.1007/3-540-18653-0_117
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