MOA 2013-BLG-127 , the SIMBAD biblio

2015ApJ...798..123J - Astrophys. J., 798, 123 (2015/January-2)

OGLE-2013-BLG-0102LA,B: microlensing binary with components at star/brown dwarf and brown dwarf/planet boundaries.

JUNG Y.K., UDALSKI A., SUMI T., HAN C., GOULD A., SKOWRON J., KOZLOWSKI S., POLESKI R., WYRZYKOWSKI L., SZYMANSKI M.K., PIETRZYNSKI G., SOSZYNSKI I., ULACZYK K., PIETRUKOWICZ P., MROZ P., KUBIAK M. (The OGLE Collaboration), ABE F., BENNETT D.P., BOND I.A., BOTZLER C.S., FREEMAN M., FUKUI A., FUKUNAGA D., ITOW Y., KOSHIMOTO N., LARSEN P., LING C.H., MASUDA K., MATSUBARA Y., MURAKI Y., NAMBA S., OHNISHI K., PHILPOTT L., RATTENBURY N.J., SAITO TO., SULLIVAN D.J., SUZUKI D., TRISTRAM P.J., TSURUMI N., WADA K., YAMAI N., YOCK P.C.M., YONEHARA A. (The MOA Collaboration), ALBROW M., CHOI J.-Y., DEPOY D.L., GAUDI B.S., HWANG K.-H., LEE C.-U., PARK H., OWEN S., POGGE R.W., SHIN I.-G., YEE J.C. (The {mu}FUN Collaboration)

Abstract (from CDS):

We present an analysis of the gravitational microlensing event OGLE-2013-BLG-0102. The light curve of the event is characterized by a strong short-term anomaly superposed on a smoothly varying lensing curve with a moderate magnification Amax∼ 1.5. It is found that the event was produced by a binary lens with a mass ratio between the components of q = 0.13 and the anomaly was caused by the passage of the source trajectory over a caustic located away from the barycenter of the binary. Based on the analysis of the effects on the light curve due to the finite size of the source and the parallactic motion of the Earth, we determine the physical parameters of the lens system. The measured masses of the lens components are M1= 0.096±0.013 M☉ and M2= 0.012±0.002 M☉, which correspond to near the hydrogen-burning and deuterium-burning mass limits, respectively. The distance to the lens is 3.04±0.31 kpc and the projected separation between the lens components is 0.80±0.08 AU.

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Journal keyword(s): binaries: general - brown dwarfs - gravitational lensing: micro

Simbad objects: 6

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