Abstract
We present line surface fluxes from the red dwarf flare star AD Leo in its quiescent state. IUE and ground-based instruments cover the UV and optical (1000–9000 Å) domains of the spectrum. The observed radiation losses from chromospheric and transition region lines amount to 4.0 * 106 erg cm−2s−1 and 2.7 * 105erg cm−2s−1, respectively. Further, from an analogy with solar active regions we estimate the total radiative energy loss in all lines formed between 25.000 K and 250.000 K to be of the order of 106 – 107 erg cm−2s−1.
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Kjeldseth-Moe, O., Andreassen, O., Maltby, P., Bartoe, J.D.F., Brueckner, G.E. and Nicolas, K.R., 1984, Adv. Space Res. 4, 8, 63.
Linsky, J.L., Bornmann P.L., Carpenter, K.G., Wing, R.F., Giampapa, M.S., Worden, S.P. and Hege, E.K., 1982, Ap.J., 260, 670.
Pettersen, B.R., and Coleman, L.A., 1981, Ap. J., 251, 571.
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© 1988 Kluwer Academic Publishers
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Sundland, S.R., Pettersen, B.R., Hawley, S.L., Kjeldseth-Moe, O., Andersen, B.N. (1988). Radiation Losses in Chromospheric and Transition Region Emission Lines from AD Leo (dM4e). In: Havnes, O., Pettersen, B.R., Schmitt, J.H.M.M., Solheim, J.E. (eds) Activity in Cool Star Envelopes. Astrophysics and Space Science Library, vol 143. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2951-7_8
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DOI: https://doi.org/10.1007/978-94-009-2951-7_8
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7827-6
Online ISBN: 978-94-009-2951-7
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