Nanase Harada

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

Nanase Harada is an Assistant Professor at the National Astronomical Observatory of Japan. Her research primarily focuses on the study of complex organic molecules and star formation in galaxies, particularly NGC 253 and NGC 1068. Recent publications include investigations into shock-induced abundance enhancements, cosmic-ray ionization rates, and the physical conditions within starburst environments. She employs advanced observational techniques, including ALCHEMI, ALMA, and HST, to explore the molecular intricacies of these cosmic phenomena.

Articles (20)

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2025

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2021

Collaborators (12)

Shunya Takekawa

Assistant Professor

Kanagawa University

JAPAN

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Tomoka Tosaki

Joetsu University of Education

JAPAN

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Fumi Egusa

University of Tokyo

JAPAN

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Takuma Izumi

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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Serena Viti

University College London

UNITED KINGDOM

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Yoshimasa Watanabe

Associate Professor

Shibaura Institute of Technology

JAPAN

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Rei Enokiya

Specially Appointed Assistant Professor

Kyushu University

JAPAN

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Jonathan Holdship

University College London

UNITED KINGDOM

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Shuro Takano

Professor

Nihon University

JAPAN

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Yoichi Tamura

Associate Professor

Nagoya University

JAPAN

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Akio Taniguchi

Project assistant professor

Nagoya University

JAPAN

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Masatoshi Imanishi

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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Nanase Harada

Research Interests

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About

Articles (20)

Complex organic molecules towards the central molecular zone of NGC 253

Shock-induced HCNH+ abundance enhancement in the heart of the starburst galaxy NGC 253 unveiled by ALCHEMI

First detection of a deuterated molecule in a starburst environment within NGC 253

Physical properties of the southwest outflow streamer in the starburst galaxy NGC 253 with ALCHEMI

Parabolic-like Trend in SiO Ratios throughout the Central Molecular Zone: Possible Signature of a Past Nuclear Activity in the Galactic Center

A Temperature or Far-ultraviolet Tracer? The HNC/HCN Ratio in M83 on the Scale of Giant Molecular Clouds

Neural Network Constraints on the Cosmic-Ray Ionization Rate and Other Physical Conditions in NGC 253 with ALCHEMI Measurements of HCN and HNC

Measuring 60 pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA

An ALCHEMI inspection of sulphur-bearing species towards the central molecular zone of NGC 253

Molecular isotopologue measurements toward super star clusters and the relation to their ages in NGC 253 with ALCHEMI

Molecular Abundance of the Circumnuclear Region Surrounding an Active Galactic Nucleus in NGC 1068 Based on an Imaging Line Survey in the 3 mm Band with ALMA

AGN-driven Cold Gas Outflow of NGC 1068 Characterized by Dissociation-sensitive Molecules

The Kiloparsec-scale Neutral Atomic Carbon Outflow in the Nearby Type 2 Seyfert Galaxy NGC 1068: Evidence for Negative AGN Feedback

Tracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253

Energizing Star Formation: The Cosmic-Ray Ionization Rate in NGC 253 Derived from ALCHEMI Measurements of H3O+ and SO

ALCHEMI Finds a “Shocking” Carbon Footprint in the Starburst Galaxy NGC 253

Deeply Buried Nuclei in the Infrared-luminous Galaxies NGC 4418 and Arp 220. I. ALMA Observations at λ = 1.4–0.4 mm and Continuum Analysis

Deeply Buried Nuclei in the Infrared-luminous Galaxies NGC 4418 and Arp 220. II. Line Forests at λ = 1.4–0.4 mm and Circumnuclear Gas Observed with ALMA

Starburst Energy Feedback Seen through HCO+/HOC+ Emission in NGC 253 from ALCHEMI

Towards the prediction of molecular parameters from astronomical emission lines using Neural Networks

Collaborators (12)

Shunya Takekawa

Tomoka Tosaki

Fumi Egusa

Takuma Izumi

Serena Viti

Yoshimasa Watanabe

Rei Enokiya

Jonathan Holdship

Shuro Takano

Yoichi Tamura

Akio Taniguchi

Masatoshi Imanishi

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