Masao Saito

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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About

Masao Saito is a Professor at the National Astronomical Observatory of Japan. His research focuses on high-mass star formation, chemical differentiation in protostars, and the observational studies of carbon-chain species utilizing ALMA and JWST. Recent publications include investigations into the initial mass function variations and the turbulent fragmentation processes in star-forming regions.

Articles (17)

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2025

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2025

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2025

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2024

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2024

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2024

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2024

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2023

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2023

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2023

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2023

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2022

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2022

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2021

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2021

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2021

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2021

Collaborators (10)

Tomomi SHIMOIKURA

Otsuma Women's University

JAPAN

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Chikako Yasui

Assistant professor

National Astronomical Observatory of Japan

UNITED STATES

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Kei Tanaka

Assistant Professor

Tokyo Institute of Technology

JAPAN

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Qizhou Zhang

Smithsonian Institution

UNITED STATES

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Kotomi Taniguchi

特任助教/Project 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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Tomoya Hirota

准教授/Associate Professor

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

JAPAN

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Fernando Olguin Choupay

Research Assistant Professor

Kyoto University

JAPAN

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Zhi-Yun Li

Professor

University of Virginia

UNITED STATES

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Shanghuo Li

Max-Planck-Institut für Astronomie

GERMANY

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Yoko Oya

Senior Lecturer

Kyoto University

JAPAN

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Masao Saito

Research Interests

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Articles (17)

Massive extended streamers feed high-mass young stars

Recent observational studies on carbon-chain species with current facilities and future prospects with ALMA & JWST

Turbulent fragmentation as the primary driver of core formation in Polaris Flare and Lupus I

Overview Results of JWST Observations of Star-forming Clusters in the Extreme Outer Galaxy

Digging into the Interior of Hot Cores with ALMA (DIHCA). IV. Fragmentation in High-mass Star-forming Clumps

The SOFIA Massive (SOMA) Star Formation Q-band follow-up

Revealing Potential Initial Mass Function Variations with Metallicity: JWST Observations of Young Open Clusters in a Low-metallicity Environment

Digging into the Interior of Hot Cores with the ALMA (DIHCA). III. The Chemical Link between NH2CHO, HNCO, and H2CO

Survey of CH3NH2 and its Formation Process

Chemical Differentiation around Five Massive Protostars Revealed by ALMA: Carbon-chain Species and Oxygen/Nitrogen-bearing Complex Organic Molecules

Mass Function of a Young Cluster in a Low-metallicity Environment. Sh 2-209

Star Formation Activity beyond the Outer Arm. II. Distribution and Properties of Star Formation

Vibrationally Excited Lines of HC3N Associated with the Molecular Disk around the G24.78+0.08 A1 Hypercompact H ii Region

Clump-scale chemistry in the NGC 2264-D cluster-forming region

Low-metallicity young clusters in the outer galaxy. III. Sh 2-127

Chemical Compositions in the Vicinity of Protostars in Ophiuchus

Carbon-chain Chemistry versus Complex-organic-molecule Chemistry in Envelopes around Three Low-mass Young Stellar Objects in the Perseus Region

Collaborators (10)

Tomomi SHIMOIKURA

Chikako Yasui

Kei Tanaka

Qizhou Zhang

Kotomi Taniguchi

Tomoya Hirota

Fernando Olguin Choupay

Zhi-Yun Li

Shanghuo Li

Yoko Oya

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