Yuta Notsu   Adam F. Kowalski   Hiroyuki Maehara   Kosuke Namekata   Kenji Hamaguchi   Teruaki Enoto   Isaiah I. Tristan   Suzanne L. Hawley   James R. A. Davenport   Satoshi Honda   Kai Ikuta   Shun Inoue   Keiichi Namizaki   Daisaku Nogami   Kazunari Shibata   
The Astrophysical Journal 961(2) 189-189 2024年1月
Abstract
We conducted the time-resolved simultaneous optical spectroscopic and photometric observations of mid-M-dwarf flare stars YZ CMi, EV Lac, and AD Leo. Spectroscopic observations were obtained using Apache Point Observatory 3.5 m and Smal...
The Astrophysical Journal 948(1) 64-64 2023年5月 [査読有り]
Abstract
Starspots and stellar flares are indicators of stellar magnetic activity. The magnetic energy stored around spots is thought to be the origin of flares, but the connection is not completely understood. To investigate the relation betwee...
The Astrophysical Journal 948(1) 9-9 2023年4月 [査読有り]
Abstract
Stellar coronal mass ejections (CMEs) have recently received much attention for their impacts on exoplanets and stellar evolution. Detecting prominence eruptions, the initial phase of CMEs, as the blueshifted excess component of Balmer ...
The Astrophysical Journal 945(1) 61-61 2023年3月 [査読有り]
<jats:title>Abstract</jats:title>
<jats:p>Active M-type stars are known to often produce superflares on the surface. Radiation from stellar (super)flares is important for exoplanet habitability, but the mechanisms are not well understood. In this...
Haining Li   Wako Aoki   Tadafumi Matsuno   Qianfan Xing   Takuma Suda   Nozomu Tominaga   Yuqin Chen   Satoshi Honda   Miho N. Ishigaki   Jianrong Shi   Jingkun Zhao   Gang Zhao   
The Astrophysical Journal 931(2) 147-147 2022年6月 [査読有り]
Abstract
We present homogeneous abundance analysis of over 20 elements for 385 very metal-poor (VMP) stars based on the LAMOST survey and follow-up observations with the Subaru Telescope. It is the largest high-resolution VMP sample (including 3...
Recently, many superflares on solar-type stars have been discovered as white-light flares (WLFs). The statistical study found a correlation between their energies (E) and durations (τ): τ ∝ E0.39, similar to those of solar hard/soft X-ray flares, ...
Publications of the Astronomical Society of Japan 69(6) 2017年12月
The first detected gravitational wave from a neutron star merger was
GW170817. In this study, we present J-GEM follow-up observations of SSS17a, an
electromagnetic counterpart of GW170817. SSS17a shows a 2.5-mag decline in the
-band from 1.7 da...
Publications of the Astronomical Society of Japan 69(6) 2017年12月
Recent detection of gravitational waves from a neutron star (NS) merger event
GW170817 and identification of an electromagnetic counterpart provide a unique
opportunity to study the physical processes in NS mergers. To derive properties
of ejected...
Publications of the Astronomical Society of Japan 69(5) 2017年10月
We present monitoring campaign observations at optical and near-infrared (NIR) wavelengths for a radio-loud active galactic nucleus (AGN) at z = 0.840, SDSS J110006.07+442144.3 (hereafter, J1100+4421), which was identified during a flare phase in ...
Tadafumi Matsuno   Wako Aoki   Timothy C. Beers   Young Sun Lee   Satoshi Honda   
Astronomical Journal 154(2) 2017年8月
We present elemental abundances for eight unevolved extremely metal-poor (EMP) stars with Teff 5500 K, among which seven have [Fe H] -3.5. The sample is selected from the Sloan Digital Sky Survey/Sloan Extension for Galactic Understanding and Expl...