activity
20112015
most citedSpectroscopically Identified Intermediate Age Stars at 0.5 - 3 pc Distance from Sgr A*

13 citations · 24 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2015★ 13 cited

Spectroscopically Identified Intermediate Age Stars at 0.5 - 3 pc Distance from Sgr A*

Shogo Nishiyama, Rainer Schoedel, Tatsuhito Yoshikawa +3

<Context.> Nuclear star clusters (NSCs) at the dynamical center of galaxies appear to have a complex star formation history. This suggests repeated star formation even in the influ…

astro-ph.GA2015★ 10 cited

Number Density Distribution of Near-Infrared Sources on a Sub-Degree Scale in the Galactic Center: Comparison with the Fe XXV Ka Line at 6.7 keV

Kazuki Yasui, Shogo Nishiyama, Tatsuhito Yoshikawa +9

The stellar distribution derived from an and -band survey of the central region of our Galaxy is compared with the Fe XXV K (6.7 keV) line intensity observed…

astro-ph.GA2014★ 1 cited

YSO search toward the boundary of the Central Molecular Zone with near-infrared polarimetry

Tatsuhito Yoshikawa, Shogo Nishiyama, Motohide Tamura +2

We have carried out near-infrared polarimetry toward the boundary of the Central Molecular Zone, in the field of (-1.4 deg -0.3 deg and 1.0 deg $\lesssim l \l…

astro-ph.GA2014

The Origin of the Galactic Center Diffuse X-ray Emission Investigated by Near-infrared Imaging and Polarimetric Observations

Shogo Nishiyama, Kazuki Yasui, Tetsuya Nagata +3

The origin of the Galactic center diffuse X-ray emission (GCDX) is still under intense investigation. We have found a clear excess in a longitudinal GCDX profile over a stellar num…

astro-ph.GA2013

Intrinsically Polarized Stars and Implication for Star Formation in the Central Parsec of Our Galaxy

Tatsuhito Yoshikawa, Shogo Nishiyama, Motohide Tamura +2

We have carried out adaptive-optics assisted observations at the Subaru telescope, and have found 11 intrinsically polarized sources in the central parsec of our Galaxy. They are s…

astro-ph.HE2013

Accretion disk and ionized absorber of the 9.7-hour dipping black hole binary MAXI J1305-704

Megumi Shidatsu, Yoshihiro Ueda, Satoshi Nakahira +14

We report the results from X-ray studies of the newly discovered black hole candidate MAXI J1305-704 based on Suzaku and Swift observations in the low/hard and high/soft states, re…