Ronin Wu, Ph.D.

Affiliations: 
2012 Physics New York University, New York, NY, United States 
Area:
General Physics, Astrophysics Physics, Astronomy and Astrophysics
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"Ronin Wu"
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Parents

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David W. Hogg grad student 2012 NYU
 (Tracing Star Formation in the Mid-infrared.)
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Publications

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Lee MY, Madden SC, Petit FL, et al. (2019) Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. II. 30 Doradus Astronomy and Astrophysics. 628
Onaka T, Nakamura T, Sakon I, et al. (2018) Near-infrared to Mid-infrared Observations of Galaxy Mergers: NGC 2782 and NGC 7727 The Astrophysical Journal. 853: 31
Wu R, Bron E, Onaka T, et al. (2018) Constraining physical conditions for the PDR of Trumpler 14 in the Carina Nebula Astronomy and Astrophysics. 618
Schirm MRP, Wilson CD, Kamenetzky J, et al. (2017) Probing the cold and warm molecular gas in the Whirlpool Galaxy: Herschel SPIRE‐FTS observations of the central region of M51 (NGC 5194) Monthly Notices of the Royal Astronomical Society. 470: 4989-5006
Fahrion K, Cormier D, Bigiel F, et al. (2017) Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C II] SOFIA/GREAT observations Astronomy and Astrophysics. 599
Fernández-Ontiveros JA, Armus L, Baes M, et al. (2017) SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust Publications of the Astronomical Society of Australia. 34
Chevance M, Madden SC, Lebouteiller V, et al. (2016) A milestone toward understanding PDR properties in the extreme environment of LMC-30 Doradus Astronomy and Astrophysics. 590
Hughes TM, Baes M, Schirm MRP, et al. (2016) The spatially resolved correlation between [N II] 205 μ m line emission and the 24 μ m continuum in nearby galaxies Astronomy and Astrophysics. 587
Hony S, Gouliermis DA, Galliano F, et al. (2015) Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC Monthly Notices of the Royal Astronomical Society. 448: 1847-1862
Wu R, Madden SC, Galliano F, et al. (2015) Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS Astronomy and Astrophysics. 575
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