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Radiation Losses in Chromospheric and Transition Region Emission Lines from AD Leo (dM4e)

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Activity in Cool Star Envelopes

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 143))

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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References

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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

  • eBook Packages: Springer Book Archive

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