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A mini-survey of ultracool dwarfs at 4.9 GHz

Antonova, A. and Doyle, G. J. and Hallinan, G. and Bourke, S. and Golden, A. (2008) A mini-survey of ultracool dwarfs at 4.9 GHz. Astronomy and Astrophysics, 487 (1). pp. 317-322. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20140205-080431873

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Abstract

Context. A selection of ultracool dwarfs are known to be radio active, with both gyrosynchrotron emission and the electron cyclotron maser instability being given as likely emission mechanisms. Aims. We explore whether ultracool dwarfs previously undetected at 8.5 GHz may be detectable at a lower frequency. Methods. We select a sample of fast rotating ultracool dwarfs with no detectable radio activity at 8.5 GHz, observing each of them at 4.9 GHz. Results. From the 8 dwarfs in our sample, we detect emission from 2MASS J07464256+2000321, with a mean flux level of 286 ±24 µJy. The light-curve of 2MASS J07464256+2000321, is dominated towards the end of the observation by a very bright, ≈100% left circularly polarized burst during which the flux reached 2.4 mJy. The burst was preceded by a raise in the level of activity, with the average flux being ≈160 µJy in the first hour of observation rising to ≈400 µJy in the 40 min before the burst. During both periods, there is significant variability. Conclusions. The detection of 100% circular polarization in the emission at 4.9 GHz points towards the electron cyclotron maser as the emission mechanism. However, the observations at 4.9 GHz and 8.5 GHz were not simultaneous, thus the actual fraction of dwarfs capable of producing radio emission, as well as the fraction of those that show periodic pulsations is still unclear, as indeed are the relative roles played by the electron cyclotron maser instability versus gyrosynchrotron emission, therefore we cannot assert if the previous non-detection at 8.5 GHz was due to a cut-off in emission between 4.9 and 8.4 GHz, or due to long term variability.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://arxiv-web3.library.cornell.edu/abs/0805.4574v1arXivDiscussion Paper
http://dx.doi.org/10.1051/0004-6361:20079275 DOIArticle
http://www.aanda.org/articles/aa/abs/2008/31/aa9275-07/aa9275-07.htmlPublisherArticle
Additional Information:© 2008 ESO. Article published by EDP Sciences. Received 19 December 2007; Accepted 3 June 2008; Published online 04 June 2008. Armagh Observatory is grant-aided by the N. Ireland Dept. of Culture, Arts & Leisure. We gratefully acknowledge the support of Science Foundation Ireland (Grant Number 07/RFP/PHYF553). This research has made use of the Simbad database, operated at CDS, Strasbourg, France.
Funders:
Funding AgencyGrant Number
Northern Ireland Department of Culture, Arts and Leisure (DCAL)UNSPECIFIED
Science Foundation Ireland07/RFP/PHYF553
Subject Keywords:stars : low-mass, brown dwarfs; radio continuum : stars; radiation mechanisms : general; masers
Issue or Number:1
Record Number:CaltechAUTHORS:20140205-080431873
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140205-080431873
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:43663
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:02 Mar 2014 14:51
Last Modified:03 Oct 2019 06:10

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