Search Results - "Maehara, Hiroyuki"
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Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data
Published in The Astrophysical journal (01-01-2021)“…We report the latest statistical analyses of superflares on solar-type (G-type main-sequence; effective temperature is 5100-6000 K) stars using all of the…”
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Do Kepler Superflare Stars Really Include Slowly Rotating Sun-like Stars?-Results Using APO 3.5 m Telescope Spectroscopic Observations and Gaia-DR2 Data
Published in The Astrophysical journal (01-05-2019)“…We report the latest view of Kepler solar-type (G-type main-sequence) superflare stars, including recent updates with Apache Point Observatory (APO) 3.5 m…”
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3
Statistical properties of superflares on solar-type stars based on 1-min cadence data
Published in Earth, planets, and space (29-04-2015)“…We searched for superflares on solar-type stars using Kepler data with 1-min sampling in order to detect superflares with a short duration. We found 187…”
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Analysis of a Kepler Light Curve of the Novalike Cataclysmic Variable KIC 8751494
Published in Publications of the Astronomical Society of Japan (25-08-2013)“…We analyzed a Kepler light curve of KIC 8751494, a recently recognized novalike cataclysmic variable in the Kepler field. We detected a stable periodicity of…”
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5
Starspot activity and superflares on solar-type stars
Published in Publications of the Astronomical Society of Japan (01-06-2017)“…Abstract We analyze the correlation between starspots and superflares on solar-type stars using observations from the Kepler mission. The analysis shows that…”
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Magnitude Estimates for the Carrington Flare in 1859 September: As Seen from the Original Records
Published in Astrophysical journal. Letters (01-09-2023)“…Abstract The Carrington flare in 1859 September is a benchmark, as the earliest reported solar flare and as an event with one of the greatest terrestrial…”
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Probable detection of an eruptive filament from a superflare on a solar-type star
Published in Nature astronomy (01-02-2022)“…Solar flares are often accompanied by filament/prominence eruptions (~10 4 K and ~10 10−11 cm −3 ), sometimes leading to coronal mass ejections that directly…”
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A Superflare on YZ Canis Minoris Observed by the Seimei Telescope and TESS: Red Asymmetry of Hα Emission Associated with White-light Emission
Published in The Astrophysical journal (01-03-2023)“…Abstract Active M-type stars are known to often produce superflares on the surface. Radiation from stellar (super)flares is important for exoplanet…”
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Starspot Mapping with Adaptive Parallel Tempering. II. Application to TESS Data for M-dwarf Flare Stars AU Microscopii, YZ Canis Minoris, and EV Lacertae
Published in The Astrophysical journal (01-05-2023)“…Abstract Starspots and stellar flares are indicators of stellar magnetic activity. The magnetic energy stored around spots is thought to be the origin of…”
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Detection of a High-velocity Prominence Eruption Leading to a CME Associated with a Superflare on the RS CVn-type Star V1355 Orionis
Published in The Astrophysical journal (01-05-2023)“…Abstract Stellar coronal mass ejections (CMEs) have recently received much attention for their impacts on exoplanets and stellar evolution. Detecting…”
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11
Temporal Evolution of Spatially Resolved Individual Star Spots on a Planet-hosting Solar-type Star: Kepler-17
Published in The Astrophysical journal (10-03-2020)“…Star spot evolution is visible evidence of the emergence/decay of the magnetic field on a stellar surface, and it is therefore important for the understanding…”
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12
Optical spectroscopic observations of a symbiotic star MWC 560 in the mass accumulation phase
Published in Publications of the Astronomical Society of Japan (01-12-2021)“…Abstract There are about a dozen symbiotic stars known to produce high-velocity jets during outbursts. MWC 560 (V694 Mon) is a symbiotic star that seems to…”
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High dispersion spectroscopy of solar-type superflare stars. II. Stellar rotation, starspots, and chromospheric activities
Published in Publications of the Astronomical Society of Japan (01-06-2015)“…We conducted high dispersion spectroscopic observations of 50 superflare stars with Subaru/HDS. These 50 stars were selected from the solar-type superflare…”
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Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares
Published in The Astrophysical journal (01-01-2024)“…Abstract Young solar-type stars frequently produce superflares, serving as a unique window into the young Sun-Earth environments. Large solar flares are…”
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15
Spectra of V1405 Cas at the Very Beginning Indicate a Low-mass ONeMg White Dwarf Progenitor
Published in The Astrophysical journal (01-12-2023)“…Abstract The lowest possible mass of ONeMg white dwarfs (WDs) has not been clarified despite its importance in the formation and evolution of WDs. We tackle…”
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Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data
Published in The Astrophysical journal (01-02-2024)“…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…”
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Time-resolved spectroscopic observations of an M-dwarf flare star EV Lacertae during a flare
Published in Publications of the Astronomical Society of Japan (01-08-2018)“…Abstract We have performed five night spectroscopic observations of the Hα line of EV Lac with a medium wavelength resolution (R ∼ 10000) using the 2 m Nayuta…”
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Calcium-rich Transient SN 2019ehk in a Star-forming Environment: Yet Another Candidate for a Precursor of a Double Neutron-star Binary
Published in The Astrophysical journal (01-05-2021)“…Abstract We present optical and near-infrared observations of SN 2019ehk, which was initially reported as a Type Ib supernova (SN). We show that it evolved to…”
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X-Ray, Optical, and Near-infrared Monitoring of the New X-Ray Transient MAXI J1820+070 in the Low/Hard State
Published in The Astrophysical journal (20-11-2018)“…We report X-ray, optical, and near-infrared monitoring of the new X-ray transient MAXI J1820+070 discovered with MAXI on 2018 March 11. Its X-ray intensity…”
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Morpho-kinematic Modeling of the Expanding Ejecta of the Extremely Slow Nova V1280 Scorpii
Published in The Astrophysical journal (01-06-2022)“…Abstract Knowledge of the morphology of nova ejecta is essential for fully understanding the physical processes involved in nova eruptions. We studied the 3D…”
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