Authors

E. Berger; G. Basri; T. A. Fleming; M. S. Giampapa; J. E. Gizis; J. Liebert; E. Martin; N. Phan-Bao;R. E. Rutledge

Comments

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Abbreviated Journal Title

Astrophys. J.

Keywords

brown dwarfs; radio continuum: stars; stars: activity; stars: low-mass; stars: magnetic fields; LOW-MASS STARS; MAIN-SEQUENCE; BROWN DWARF; SOLAR NEIGHBORHOOD; ROSAT; SURVEY; COOL STARS; MID-M; EMISSION; ROTATION; FLARE; Astronomy & Astrophysics

Abstract

As part of our on-going investigation into the magnetic field properties of ultracool dwarfs, we present simultaneous radio, X-ray, and H alpha observations of three M9.5-L2.5 dwarfs (BRI 0021-0214, LSR 060230.4+391059, and 2MASS J052338.2-140302). We do not detect X-ray or radio emission from any of the three sources, despite previous detections of radio emission from BRI 0021 and 2M0523-14. Steady and variable H alpha emission are detected from 2M0523-14 and BRI 0021, respectively, while no H alpha emission is detected from LSR 0602+39. Overall, our survey of nine M8-L5 dwarfs doubles the number of ultracool dwarfs observed in X-rays, and triples the number of L dwarfs, providing in addition the deepest limits to date, log (L-X/L-bol) less than or similar to -5. With this larger sample we find the first clear evidence for a substantial reduction in X-ray activity, by about two orders of magnitude, from mid-M to mid-L dwarfs. We find that the decline in H alpha roughly follows LH alpha/L-bol proportional to 10(-0.4x(SP-6)) for SP > = 6, where SP = 0 for spectral type M0. In the radio band, however, the luminosity remains relatively unchanged from M0 to L4, leading to a substantial increase in L-rad/L-bol. Our survey also provides the first comprehensive set of simultaneous radio/X-ray/H alpha observations of ultracool dwarfs, and reveals a clear breakdown of the radio/X-ray correlation beyond spectral type M7, evolving smoothly from L-nu,L-rad/L-X approximate to 10(-15.5) to similar to 10(-11.5) Hz(-1) over the narrow spectral-type range M7-M9. This breakdown reflects the substantial reduction in X-ray activity beyond M7, but its physical origin remains unclear since, as evidenced by the uniform radio emission, there is no drop in the field dissipation and particle acceleration efficiency. Based on the results of our survey, we conclude that a further investigation of magnetic activity in ultracool dwarfs will benefit from a two-pronged approach: multi-rotation observations of nearby known active sources and a snapshot survey of a large sample within similar to 50 pc to uncover rare flaring objects.

Journal Title

Astrophysical Journal

Volume

709

Issue/Number

1

Publication Date

1-1-2010

Document Type

Article

Language

English

First Page

332

Last Page

341

WOS Identifier

WOS:000273282500030

ISSN

0004-637X

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