XMM-Newton observations of the nearby brown dwarf LP 944-20
Preprint
- 16 October 2002
Abstract
The nearby (d=5.0 pc) brown dwarf LP944-20 was observed with the XMM-Newton satellite on 07 January 2001. The target was detected with the Optical Monitor (V=16.736$\pm$0.081), but it was not detected during the $\approx 48$ ks observation with the X-ray telescopes. We determine a $3\sigma$ upper limit for the X-ray emission from this object of $L_{X}-$2.5] are very rare (less than 0.7% of the time). Flares like the one detected by Chandra [Log$(L_X/L_{bol})=-$4.1] have a duty cycle of about 6%, which is lower than the radio flare duty cycle ($\sim$13%). When compared with other M dwarfs, LP944-20 appears to be rather inactive in X-rays despite of its relative youth, fast rotation and its moderately strong activity at radio wavelengths.
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All Related Versions
- Version 1, 2002-10-16, ArXiv
- Published version: New Astronomy, 7 (8), 595.
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