output
20062009
most citedDiscovery of a Jupiter/Saturn Analog with Gravitational Microlensing

366 citations

Showing 2008Show all

13 papers · 1 filter

astro-ph200827 cited

Distinguishing between Planetary and Binary Interpretations of Microlensing Central Perturbations under Severe Finite-Source Effect

Cheongho Han

In the current strategy of microlensing planet searches focusing on high-magnification events, wide and close binaries pose important sources of contamination that imitates planeta…

astro-ph2008224 cited

The sdB+M Eclipsing System HW Virginis and its Circumbinary Planets

Jae Woo Lee, Seung-Lee Kim, Chun-Hwey Kim +4

For the very short-period sdB eclipsing binary HW Vir, we present new CCD photometry made from 2000 through 2008. In order to obtain consistency of the binary parameters, our new l…

astro-ph200817 cited

Nova-Like Cataclysmic Variable TT Ari: QPO Behaviour Coming Back From Positive Superhumps

Y. Kim, I. L. Andronov, S. M. Cha +1

We study the variability of the nova-like cataclysmic variable TT Ari, on time-scales of between minutes and months. The observations in the filter R were obtained at the 40-cm tel…

cond-mat.other20088 cited

Current-Induced Resonant Motion of a Magnetic Vortex Core: Effect of Nonadiabatic Spin Torque

Jung-Hwan Moon, Dong-Hyun Kim, Myung Hwa Jung +1

The current-induced resonant excitation of a magnetic vortex core is investigated by means of analytical and micromagnetic calculations. We find that the radius and the phase shift…

astro-ph20083 cited

Limits of Binaries That Can Be Characterized by Gravitational Microlensing

Doeon Kim, Yoon-Hyun Ryu, Byeong-Gon Park +5

Due to the high efficiency of planet detections, current microlensing planet searches focus on high-magnification events. High-magnification events are sensitive to remote binary c…

astro-ph200833 cited

Detection of Fluorine in the Halo Planetary Nebula BoBn 1: Evidence For a Binary Progenitor Star

Masaaki Otsuka, Hideyuki Izumiura, Akito Tajitsu +1

We have found the fluorine lines [F IV] 3996.92A,4059.90A in the extremely metal-poor ([Ar/H] = -2.10+/-0.21) halo planetary nebula (PN) BoBn 1 in high-dispersion spectra from the…