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Substructures in the Disk-forming Region of the Class 0 Low-mass Protostellar Source IRAS 16293−2422 Source A on a 10 au Scale

The Astrophysical journal, 2020-12, Vol.904 (2), p.185

2020

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Chemical Variation among Protostellar Cores: Dependence on Prestellar Core Conditions

The Astrophysical journal, 2020-07, Vol.897 (2), p.110

2020

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Synthetic Observations of the Infalling Rotating Envelope: Links between the Physical Structure and Observational Features

The Astrophysical journal, 2024-01, Vol.961 (1), p.31

2024

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Sub-arcsecond Kinematic Structure of the Outflow in the Vicinity of the Protostar in L483

The Astrophysical journal, 2018-08, Vol.863 (1), p.72

2018

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Molecular Distributions of the Protostellar Envelope and the Outflow of IRAS 15398-3359: Principal Component Analysis

The Astrophysical journal, 2020-09, Vol.900 (1), p.40

2020

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Complex Organic Molecules in Taurus Molecular Cloud-1

The Astrophysical journal, 2018-02, Vol.854 (2), p.116

2018

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The Perseus ALMA Chemistry Survey (PEACHES). I. The Complex Organic Molecules in Perseus Embedded Protostars

The Astrophysical journal, 2021-03, Vol.910 (1), p.20

2021

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L483: Warm Carbon-chain Chemistry Source Harboring Hot Corino Activity

The Astrophysical journal, 2017-03, Vol.837 (2), p.174

2017

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Chemical Differentiation and Temperature Distribution on a Few au Scale around the Protostellar Source B335

The Astrophysical journal, 2022-08, Vol.935 (2), p.136

2022

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Molecular-cloud-scale Chemical Composition. III. Constraints of Average Physical Properties through Chemical Models

The Astrophysical journal, 2019-02, Vol.871 (2), p.238

2019

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Molecular Distributions of the Disk/Envelope System of L483: Principal Component Analysis for the Image Cube Data

The Astrophysical journal, 2021-12, Vol.923 (2), p.168

2021

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SPECTRAL LINE SURVEY TOWARD A MOLECULAR CLOUD IN IC10

The Astrophysical journal, 2016-10, Vol.829 (2), p.94

2016

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Laboratory Measurement of CH2DOH Line Intensities in the Millimeter-wave Region

The Astrophysical journal, 2023-11, Vol.957 (1), p.4

2023

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Rotating Motion of the Outflow of IRAS 16293-2422 A1 at Its Origin Point Near the Protostar

The Astrophysical journal, 2021-11, Vol.921 (1), p.12

2021

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SPECTRAL LINE SURVEY TOWARD MOLECULAR CLOUDS IN THE LARGE MAGELLANIC CLOUD

The Astrophysical journal, 2016-02, Vol.818 (2), p.161

2016

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GEOMETRIC AND KINEMATIC STRUCTURE OF THE OUTFLOW/ENVELOPE SYSTEM OF L1527 REVEALED BY SUBARCSECOND-RESOLUTION OBSERVATION OF CS

The Astrophysical journal, 2015-10, Vol.812 (1), p.1-12

2015

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Discovery of the Second Warm Carbon-Chain-Chemistry Source, IRAS15398 – 3359 in Lupus

The Astrophysical journal, 2009-05, Vol.697 (1), p.769-786

2009

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Temperature Structure of the Pipe Nebula Studied by the Intensity Anomaly of the OH 18 cm Transition

The Astrophysical journal, 2020-12, Vol.904 (2), p.136

2020

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Sulfur-bearing Species Tracing the Disk/Envelope System in the Class I Protostellar Source Elias 29

The Astrophysical journal, 2019-08, Vol.881 (2), p.112

2019

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The Effect of Far-infrared Radiation on the Hyperfine Anomaly of the OH 18 cm Transition

The Astrophysical journal, 2019-01, Vol.871 (1), p.89

2019

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ALMA Observations of the IRDC Clump G34.43+00.24 MM3: Complex Organic and Deuterated Molecules

The Astrophysical journal, 2018-04, Vol.857 (1), p.35

2018

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MOLECULAR DISTRIBUTION IN THE SPIRAL ARM OF M51

The Astrophysical journal, 2016-03, Vol.819 (2), p.144

2016

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Long Carbon Chains in the Warm Carbon-chain-chemistry Source L1527: First Detection of C7H in Molecular Clouds

The Astrophysical journal, 2017-09, Vol.847 (1)

2017

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Abundant Carbon-Chain Molecules toward the Low-Mass Protostar IRAS 04368+2557 in L1527

The Astrophysical journal, 2008-01, Vol.672 (1), p.371-381

2008

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The Chemical Nature of Orion Protostars: Are ORANGES Different from PEACHES? ORANGES II

The Astrophysical journal, 2022-04, Vol.929 (1), p.10

2022

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Substructures in the Disk-forming Region of the Class 0 Low-mass Protostellar Source IRAS 16293−2422 Source A on a 10 au Scale

Chemical Variation among Protostellar Cores: Dependence on Prestellar Core Conditions

Synthetic Observations of the Infalling Rotating Envelope: Links between the Physical Structure and Observational Features

Sub-arcsecond Kinematic Structure of the Outflow in the Vicinity of the Protostar in L483

Molecular Distributions of the Protostellar Envelope and the Outflow of IRAS 15398-3359: Principal Component Analysis

Complex Organic Molecules in Taurus Molecular Cloud-1

The Perseus ALMA Chemistry Survey (PEACHES). I. The Complex Organic Molecules in Perseus Embedded Protostars

L483: Warm Carbon-chain Chemistry Source Harboring Hot Corino Activity

Chemical Differentiation and Temperature Distribution on a Few au Scale around the Protostellar Source B335

Molecular-cloud-scale Chemical Composition. III. Constraints of Average Physical Properties through Chemical Models

Molecular Distributions of the Disk/Envelope System of L483: Principal Component Analysis for the Image Cube Data

SPECTRAL LINE SURVEY TOWARD A MOLECULAR CLOUD IN IC10

Laboratory Measurement of CH2DOH Line Intensities in the Millimeter-wave Region

Rotating Motion of the Outflow of IRAS 16293-2422 A1 at Its Origin Point Near the Protostar

SPECTRAL LINE SURVEY TOWARD MOLECULAR CLOUDS IN THE LARGE MAGELLANIC CLOUD

GEOMETRIC AND KINEMATIC STRUCTURE OF THE OUTFLOW/ENVELOPE SYSTEM OF L1527 REVEALED BY SUBARCSECOND-RESOLUTION OBSERVATION OF CS

Discovery of the Second Warm Carbon-Chain-Chemistry Source, IRAS15398 – 3359 in Lupus

Temperature Structure of the Pipe Nebula Studied by the Intensity Anomaly of the OH 18 cm Transition

Sulfur-bearing Species Tracing the Disk/Envelope System in the Class I Protostellar Source Elias 29

The Effect of Far-infrared Radiation on the Hyperfine Anomaly of the OH 18 cm Transition

ALMA Observations of the IRDC Clump G34.43+00.24 MM3: Complex Organic and Deuterated Molecules

MOLECULAR DISTRIBUTION IN THE SPIRAL ARM OF M51

Long Carbon Chains in the Warm Carbon-chain-chemistry Source L1527: First Detection of C7H in Molecular Clouds

Abundant Carbon-Chain Molecules toward the Low-Mass Protostar IRAS 04368+2557 in L1527

The Chemical Nature of Orion Protostars: Are ORANGES Different from PEACHES? ORANGES II

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