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Yu-Hsuan Teng
Yu-Hsuan Teng
University of California, San Diego
Astrophysics
Physics
Molecular cloud
Kinematics
Astronomy
4
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14
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Molecular Gas Properties and CO-to-$\mathrm{H_2}$ Conversion Factors in the Central Kiloparsec of NGC 3351.
2021
arXiv: Astrophysics of Galaxies
Yu-Hsuan Teng
Karin Sandstrom
Jiayi Sun
Adam K. Leroy
L. Clifton Johnson
Alberto D. Bolatto
J. M. Diederik Kruijssen
Andreas Schruba
Antonio Usero
Ashley T. Barnes
Frank Bigiel
Guillermo A. Blanc
Brent Groves
Frank P. Israel
Daizhong Liu
Erik Rosolowsky
Eva Schinnerer
J.-D. T. Smith
Fabian Walter
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Physical Conditions and Kinematics of the Filamentary Structure in Orion Molecular Cloud 1
2020
The Astrophysical Journal
Yu-Hsuan Teng
Naomi Hirano
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Physical Conditions and Kinematics of the Filamentary Structure in Orion Molecular Cloud 1
2020
The Astrophysical Journal
Yu-Hsuan Teng
Naomi Hirano
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Physical Conditions and Kinematics of the Filamentary Structure in Orion Molecular Cloud 1
2020
arXiv: Astrophysics of Galaxies
Yu-Hsuan Teng
Naomi Hirano
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Citations (2)
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