Abstract
We explore the radio emission from the M9 dwarf, TVLM513-46546, at multiple radio frequencies, determining the flux spectrum of persistent radio emission, as well as constraining the levels of circular polarization. Detections at both 3.6 and 6 cm provide spectral index measurement $\alpha$ (where S$_{u} \propto u^{\alpha}$) of $-0.4\pm0.1$. A detection at 20 cm suggests that the spectral peak is between 1.4 and 5 GHz. The most stringent upper limits on circular polarization are at 3.6 and 6 cm, with $V/I
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CITATION STYLE
Osten, R. A., Hawley, S. L., Bastian, T. S., & Reid, I. N. (2006). The Radio Spectrum of TVLM 513‐46546: Constraints on the Coronal Properties of a Late M Dwarf. The Astrophysical Journal, 637(1), 518–521. https://doi.org/10.1086/498345
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