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WISE J072003.20-084651.2: AN OLD AND ACTIVE M9.5 + T5 SPECTRAL BINARY 6 pc FROM THE SUN
We report observations of the recently discovered, nearby late-M dwarf WISE J072003.20-084651.2. With high-resolution optical and near-infrared spectroscopy, we measure a stable radial velocity of +83.8 + or - 0.3 km s super(-1), indicative of old disk kinematics and consistent with the angular sepa...
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Published in: | The Astronomical journal 2015-03, Vol.149 (3), p.1-17 |
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Main Authors: | , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | We report observations of the recently discovered, nearby late-M dwarf WISE J072003.20-084651.2. With high-resolution optical and near-infrared spectroscopy, we measure a stable radial velocity of +83.8 + or - 0.3 km s super(-1), indicative of old disk kinematics and consistent with the angular separation of the possible companion. We measure a projected rotational velocity of v sin i = 8.0 + or - 0.5 km s super(-1) and find evidence of low-level variabilty (~1.5%) in a 13 day TRAPPIST light curve, but cannot robustly constrain the rotational period. We also observe episodic changes in brightness (1%-2%) and occasional flare bursts (4%-8%) with a 0.8% duty cycle, and order-of-magnitude variations in H alpha line strength. Combined, these observations reveal WISE J0720-0846 to be an old, very low-mass binary whose components straddle the hydrogen burning minimum mass, and whose primary is a relatively rapid rotator and magnetically active. |
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ISSN: | 1538-3881 0004-6256 1538-3881 |
DOI: | 10.1088/0004-6256/149/3/104 |