Miho N. Ishigaki

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助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

Japan

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About

Miho N. Ishigaki is an Assistant Professor at the National Astronomical Observatory of Japan. His research focuses on the structural and chemical properties of globular clusters, as well as the evolution of stellar populations in galaxies. Recent articles include studies on chemical abundances in stellar streams and the chemo-dynamical evolution of simulated galaxies. He is actively contributing to the understanding of galactic formation and stellar dynamics.

Recent Grants

Grant: Close

The formation of the Milky Way halo probed by statistical samples of elemental abundances in metal-poor stars

Open Date: 2017-04-01

Close Date: 2020-03-01

Grant: Close

Revealing the early phase of the Milky Way Formation based on chemical abundances in globular clusters

Open Date: 2011-04-01

Close Date: 2012-03-01

Miho N. Ishigaki

Research Interests

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About

Recent Grants

Articles (18)

Chemical Abundances of Seven Stars in the GD-1 Stream

Th/Eu abundance ratio of red giants in the Kepler field

Constructing a Pristine View of Extended Globular Cluster Structure

A pristine view of galactic globular clusters and their peripheries: Omega Centauri

EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4–10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models

Chemo-dynamical Evolution of Simulated Satellites for a Milky Way–like Galaxy

Detection of a Spatially Extended Stellar Population in M33: A Shallow Stellar Halo?

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties

Cerium Features in Kilonova Near-infrared Spectra: Implication from a Chemically Peculiar Star

Machine Learning Detects Multiplicity of the First Stars in Stellar Archaeology Data

Transition Probabilities of Near-infrared Ce iii Lines from Stellar Spectra: Applications to Kilonovae

Existence of tidal tails for the globular cluster NGC 5824

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances

Revisit NGC 5466 tidal stream with Gaia, SDSS/SEGUE, and LAMOST

Top-heavy stellar mass distribution in galactic nuclei inferred from the universally high abundance ratio of [Fe/Mg]

Origin of metals in old Milky Way halo stars based on GALAH and Gaia

Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances*

Collaborators (21)

Kimihiko Nakajima

Yutaka Komiyama

Chiaki Kobayashi

Wako Aoki

Jae-Joon Lee

Tilman Hartwig

Ken’ichi Nomoto

Nozomu Tominaga

Rosemary Wyse

Takanobu Kirihara

Puragra Guhathakurta

Takuma Suda

Koh Takahashi

Norbert Christlieb

Kohei Hayashi

Akihiro Suzuki

Daiji Kato

Takayuki Saitoh

Evan Kirby

Shing Chi Leung

Masao Takata

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