Wako Aoki

教授/Professor

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

Japan

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Wako Aoki is a Professor at the National Astronomical Observatory of Japan. His research focuses on chemical abundances in stars, particularly metal-poor stars, and their implications for stellar evolution and nucleosynthesis. Recent articles include studies on elemental abundances and actinide-boost stars, advancing the understanding of very metal-poor stellar populations.

Articles (20)

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2025

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2022

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2022

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2022

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2021

Collaborators (13)

Miho N. Ishigaki

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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Takashi Okamoto

Professor

Hokkaido University

JAPAN

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Jae-Joon Lee

Korea Advanced Institute of Science and Technology

SOUTH KOREA

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Motohide TAMURA

特任教授/Project Professor

自然科学研究機構アストロバイオロジーセンター/National Institutes of Natural Sciences, Astrobiology Center

JAPAN

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Nozomu Tominaga

Professor

National Astronomical Observatory of Japan

JAPAN

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Yasunori Hori

Associate professor

Okayama University

JAPAN

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Takuma Suda

Lecturer

University of Tokyo

JAPAN

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Junichiro Makino

Kobe University

JAPAN

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Norbert Christlieb

Professor

Ruprecht Karls Universität Heidelberg

GERMANY

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Daiji Kato

教授/Professor

核融合科学研究所/National Institute for Fusion Science

JAPAN

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Alexander Heger

Professor

MONASH UNIVERSITY

AUSTRALIA

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Teruyuki Hirano

National Institutes of Natural Sciences

JAPAN

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Masao Takata

University of Tokyo

JAPAN

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Wako Aoki

Research Interests

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Articles (20)

Revisiting Near-infrared Features of Kilonovae: The Importance of Gadolinium

Chemical Abundances of Seven Stars in the GD-1 Stream

Detailed chemical abundance analysis of metal-poor turn-off stars: One with [Fe/H] &lt; –4 and three with [Fe/H] &lt; –3

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

Elemental abundances of 44 very metal-poor stars determined from Subaru/IRD near-infrared spectra

An Actinide-boost Star Discovered in the Gaia-Sausage-Enceladus

A Systematic NLTE Study of Very Metal-poor Stars with Metallicity down to −4.3 dex. I. Global Stellar Parameters Based on High-resolution Spectra

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

Detection of the Actinide Th in an r-process-enhanced Star with Accretion Origin

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

Unique Chemical Composition of the Very Metal-poor Star LAMOST J1645+4357

A metal-poor star with abundances from a pair-instability supernova

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

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

Elemental Abundances of nearby M Dwarfs Based on High-resolution Near-infrared Spectra Obtained by the Subaru/IRD Survey: Proof of Concept

Gaia DR2 and EDR3 data and evolutionary status of post-AGB stars with high radial velocities

Origin of highly r-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy

Silicon and strontium abundances of very metal-poor stars determined from near-infrared spectra

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

Collaborators (13)

Miho N. Ishigaki

Takashi Okamoto

Jae-Joon Lee

Motohide TAMURA

Nozomu Tominaga

Yasunori Hori

Takuma Suda

Junichiro Makino

Norbert Christlieb

Daiji Kato

Alexander Heger

Teruyuki Hirano

Masao Takata

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Detailed chemical abundance analysis of metal-poor turn-off stars: One with [Fe/H] < –4 and three with [Fe/H] < –3