We present the analysis of KMT-2016-BLG-0212, a low flux-variation (Iflux−var ∼ 20 mag) microlensing event, which is in a high-cadence (Γ = 4hr −1) field of the three-telescope Korea Microlensing Telescope Network (KMTNet) survey. The event shows a short anomaly that is incompletely covered due to the brief visibility intervals that characterize the early microlensing season when the anomaly occurred. We show that the data are consistent with two classes of solutions, characterized respectively by low-mass brown-dwarf (q = 0.037) and sub-Neptune (q < 10−4) companions. Future high-resolution imaging should easily distinguish between these solutions.

Following the 2008 financial crisis, globalized markets in North America and Europe experience a shift in public opinion toward a renunciation of globalization and a reorientation toward traditional (domestic) values. Responding to this paradigm change, multi-national corporations (MNCs) face the decision of whether (a) to continue to pursue global branding strategies or (b) to align their global brands with local consumer cultures. This decision requires an understanding of how the degree of market globalization relates to consumer preferences. The present study draws on signaling theory to empirically investigate (a) the relative impact of a brand’s globalness (i.e., perceived brand globalness) and its cultural market alignment (i.e., perceived cultural symbolism) in eliciting perceptions of brand credibility and brand quality (b) across two countries that differ regarding their degree of market globalization (Germany and South Korea). Findings indicate that the signaling value of global brands, as a function of their market reach, is greater in globalizing markets than in globalized markets, whereas the signaling value associated with cultural market alignment is greater in globalized markets than in globalizing markets. Implications of the findings for theory and practice are considered.

We report the characterization of a massive (mp = 3:91:4Mjup) microlensing planet (OGLE- 2015-BLG-0954Lb) orbiting an M dwarf host (M = 0:33  0:12M) at a distance toward the Galactic bulge of 0:6+0:4 􀀀0:2 kpc, which is extremely nearby by microlensing standards. The planet-host projected separation is a?  1:2AU. The characterization was made possible by the wide-eld (4 deg2) high cadence (􀀀 = 6 hr􀀀1) monitoring of the Korea Microlensing Telescope Network (KMTNet), which had two of its three telescopes in commissioning operations at the time of the planetary anomaly. The source crossing time t = 16 min is among the shortest ever published. The high-cadence, wide-eld observations that are the hallmark of KMTNet are the only way to routinely capture such short crossings. High-cadence resolution of short caustic crossings will preferentially lead to mass and distance measurements for the lens. This is because the short crossing time typically implies a nearby lens, which enables the measurement of additional eects (bright lens and/or microlens parallax). When combined with the measured crossing time, these eects can yield planet/host masses and distance.

The slow evolution of global magnetic fields and other dynamical processes in atmospheres of CP magnetic stars lead to the development of induced electric currents in all conductive atmospheric layers. The Lorentz force, which results from the interaction between a magnetic field and the induced currents, may modify the atmospheric structure and provide insight into the formation and evolution of stellar magnetic fields. This modification of the pressure-temperature structure influences the formation of absorption spectral features producing characteristic rotational variability of some spectral lines, especially the Balmer lines (Valyavin et al., 2004 and references therein). In order to study these theoretical predictions we began systematic spectroscopic survey of Balmer line variability in spectra of brightest CP magnetic stars. Here we present the first results of the program. A0p star ⊝ Aur revealed significant variability of the Balmer profiles during the star's rotation. Character of this variablity corresponds to that classified by Kroll (1989) as a result of an impact of significant Lorentz force. From the obtained data we estimate that amplitudes of the variation at Hα, Hβ, Hɤ and Hδ profiles reach up to 2.4%during full rotation cycle of the star. Using computation of our model atmospheres (Valyavin et al., 2004) we interpret these data within the framework of the simplest model of the evolution of global magnetic fields in chemically peculiar stars. Assuming that the field is represented by a dipole, we estimate the characteristic e.m.f. induced by the field decay electric current (and the Lorentz force as the result) on the order of E ~ 10 -11 cgs units, which may indicate very fast (< < 1010 years) evolution rate of the field. This result strongly contradicts the theoretical point of view that global stellar magnetic fields of CP stars are fossil and their the characteristic decay time of about 1010 yr. Alternatively, we briefly discuss concurring effects (like the ambipolar diffusion) which may also lead to significant atmospheric currents producing the observable Lorentz force.

1981년부터 최 등이 재래종 옥수수의 수집종 가운데서 병발한 한계통(MET)을 분얼이 많이되고 또한 개체당 이삭(수)수도 많아서 사료용 옥수수의 육종재료로 가치가 있다고 생각되었으나 이 옥수수에 대한 유전적 분석이 확실히 되어 있지를 않았다. 따라서 본연구에서는 MET와 비분얼성이며 이삭도 하나 밖에 달리지 않는 수원 19호 (Mo17 B68) 교잡종을 이용하여 F1 , F2 , BC1 , 세대를 양성하고 Mather의 세대평균분석법에 의하여 분석한 결과 MET 계통의 다수.다얼성은 염색체상의 유전인자에 의한 다기 보다 세포질적 유전인자에 의한다는 것을 확인하였다. 이같은 결론은 MET계통을 모계로 하여 교잡한 려잡종 세대에서 확실히 얻을 수가 있었다. 즉 MET 계통을 모계로 이용했을 때의 평균분얼과 이삭수는 MET를 부계로 이용했을 때의 분얼수와 이삭수 보다 많았는데 이는 이같은 특성들이 모계유전을 하기 때문이다. 그러나 이같은 특성들이 F1 이나 F2 에서 나타나지 않은 것은 F1 에서 특히 보여주는 잡종강세현상 때문에 옥수수의 정부우세성이 매우커서 상반적으로 분얼이나 이삭의 발달이 억제되었기 때문이라고 생각된다. 그리고 분얼이나 이삭의 절대수가 모계로 이용했던 MET에서 보다 잡종세대가 진전될수록 적어지는 것은 잡종강세외에도 MET계통의 세포질약 내지 유전인자적 축적량(Dose)이 적어지기 때문이라고 생각되어진다. 이같은 MET계통의 특성은 려교잡에 의한 MET계통의 세포질을 유지하거나 축적하므로써 사료용 옥수수의 육종에 이용될 수 있을 것으로 보여졌다.에서 조생종이 높은 발아력을 나타냈으나 16℃ 에서는 조, 중, 만생종 간에 발아력 차이가 없었다. 5. 참깨 종자중과 발아율과의 관계는 단일품종 내에서는 종자중이 무거울수록 발아율이 높았으며 평균 발아일수도 단축되는 경향을 보였으나 공시품종들의 천립중의 경중 특성에 따른 발아력 차이는 없었다.e more the silica filler was added, and the lower the gel temperature was in the epoxy system. In this study it is concluded that the curing of the silica filled epoxy system was found to be accelerated, as silica was added to the epoxy compound.ed by adults who are middle-aged or elderly. If altered colors are applied to the digital products as much as popular culture changes, it can assist the elderly with their weakened physical abilities.동위효소 사이의 특성을 나타냈고, 골격근과 눈 조직에서 피루브산에 대한 LDH의 친화력이 상당히 크므로 LDH가 혐기적 조건에서 효율적으로 기능을 하는 것으로 사료된다.5) and "Cleanliness of clothes ＆ features" (p ＜0.05) of VIP ward were significantly higher than those of a general ward.tive to apply.아울러 고려(考慮)해야 한다. 이것