Slowly Varying Component of Radio Emission from TVLM 513-46546 and Continuous Sources of High Energy Electrons in the Coronae of UltraCool Stars
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Geophysics
Link
http://link.springer.com/article/10.1134/S0016793218080212/fulltext.html
Reference11 articles.
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2. Dulk, G.A., Radio emission from the Sun and stars, Ann. Rev. Astron. Astrophys., 1985, vol. 23, pp. 169–224.
3. Guedel, M. and Benz, A.O., Similar X-ray/microwave ratios in solar flares and coronae of active stars, Astrophys. J., 1993, vol. 405, pp. L63–L66.
4. Hallinan, G., Bourke, S., Lane, C., Antonova, A., Zavala, R.T., Brisken, W.F., Boyle, R.P., Vrba, F.J., Doyle, J.G., and Golden, A., Periodic bursts of coherent radio emission from an ultracool dwarf, Astrophys. J. Lett., 2007, vol. 663, pp. L25–L28.
5. Osten, R.A., Hawley, S.L., Bastian, T.S., and Reid, I.N., The radio spectrum of TVLM 513-46546: Constraints on the coronal properties of a late M dwarf, Astrophys. J., 2006, vol. 637, pp. 518–521.
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