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Auroral radio emission from late L and T dwarfs: A new constraint on dynamo theory in the substellar regime

Kao, Melodie M. and Hallinan, Gregg and Pineda, J. Sebastian and Escala, Ivanna and Burgasser, Adam and Bourke, Stephen and Stevenson, David (2016) Auroral radio emission from late L and T dwarfs: A new constraint on dynamo theory in the substellar regime. Astrophysical Journal, 818 (1). Art. No. 24. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20160314-093014878

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Abstract

We have observed six late L and T dwarfs with the Karl G. Jansky Very Large Array (VLA) to investigate the presence of highly circularly polarized radio emission, associated with large-scale auroral currents. Previous surveys encompassing ~60 L6 or later targets have yielded only one detection. Our sample includes the previously detected T6.5 dwarf 2MASS 10475385+2124234, as well as five new targets selected for the presence of Hα emission and/or optical infrared photometric variability, which are possible manifestations of auroral activity. We detect 2MASS 10475385+2124234, as well as four of the five targets in our biased sample, including the strong IR-variable source SIMP J01365662+0933473 and bright Hα emitter 2MASS 12373919+6526148, reinforcing the possibility that activity at these disparate wavelengths is related. The radio emission frequency corresponds to a precise determination of the lower-bound magnetic field strength near the surface of each dwarf, and this new sample provides robust constraints on dynamo theory in the low-mass brown dwarf regime. Magnetic fields ≳2.5 kG are confirmed for five of six targets. Our results provide tentative evidence that the dynamo operating in this mass regime may be inconsistent with predicted values from a recently proposed model. Further observations at higher radio frequencies are essential for verifying this assertion.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.3847/0004-637X/818/1/24DOIArticle
http://iopscience.iop.org/article/10.3847/0004-637X/818/1/24/metaPublisherArticle
http://arxiv.org/abs/1511.03661arXivDiscussion Paper
ORCID:
AuthorORCID
Kao, Melodie M.0000-0001-5125-1414
Hallinan, Gregg0000-0002-7083-4049
Pineda, J. Sebastian0000-0002-4489-0135
Escala, Ivanna0000-0002-9933-9551
Burgasser, Adam0000-0002-6523-9536
Stevenson, David0000-0001-9432-7159
Additional Information:© 2016 American Astronomical Society. Received 2015 June 25; accepted 2015 November 18; published 2016 February 4. M.M.K. thanks Jackie Villadsen, E. Sterl Phinney, Ulrich Christensen, and Shri Kulkarni for illuminating and helpful conversations. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. J.S.P. was supported by a grant from the National Science Foundation Graduate Research Fellowship under grant no. DGE-1144469.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
Associated Universities, Inc.UNSPECIFIED
NSF Graduate Research FellowshipDGE-1144469
Subject Keywords:brown dwarfs; planets and satellites: aurorae; planets and satellites: magnetic fields; radio continuum: stars; stars: individual (SIMP J01365662+0933473) ; stars: magnetic field
Issue or Number:1
Record Number:CaltechAUTHORS:20160314-093014878
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160314-093014878
Official Citation:Melodie M. Kao et al 2016 ApJ 818 24
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:65327
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:14 Mar 2016 18:29
Last Modified:06 Feb 2020 23:40

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