Ghent University Academic Bibliography

Your filters: cql: author="Williams, Thomas G." or (type any "bookEditor issueEditor" and editor="Williams, Thomas G.")

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Dynamical resonances in PHANGS galaxies

Marina Ruiz-García, Miguel Querejeta, Santiago García-Burillo, Eric Emsellem, Sharon Meidt van der Wel (UGent) , Mattia C. Sormani, Eva Schinnerer, Thomas G. Williams, Zein Bazzi, Dario Colombo, et al.

(2024) ASTRONOMY & ASTROPHYSICS. 691.
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Simulating nearby disc galaxies on the main star formation sequence : I. Bar formation and the building of the central gas reservoir

Pierrick Verwilghen, Eric Emsellem, Florent Renaud, Milena Valentini, Jiayi Sun, Sarah Jeffreson, Ralf S. Klessen, Mattia C. Sormani, Ashley T. Barnes, Klaus Dolag, et al.

(2024) ASTRONOMY & ASTROPHYSICS. 687.
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Neutral atomic and molecular gas dynamics in the nearby spiral galaxies NGC 1512, NGC 4535, and NGC 7496

Sebastian Laudage, Cosima Eibensteiner, Frank Bigiel, Adam K. Leroy, Sharon Meidt van der Wel (UGent) , Eva Schinnerer, W. J. G. de Blok, Miguele Querejeta, Sophia Stuber, Dario Colombo, et al.

(2024) ASTRONOMY & ASTROPHYSICS. 690.
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A 260 pc resolution ALMA map of HCN(1–0) in the galaxy NGC 4321

Lukas Neumann, Frank Bigiel, Ashley T. Barnes, Molly J. Gallagher, Adam Leroy, Antonio Usero, Erik Rosolowsky, Ivana Bešlić, Médéric Boquien, Yixian Cao, et al.

(2024) ASTRONOMY & ASTROPHYSICS. 691.
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A two-component probability distribution function describes the mid-IR emission from the disks of star-forming galaxies

Debosmita Pathak, Adam K. Leroy, Todd A. Thompson, Laura A. Lopez, Francesco Belfiore, Médéric Boquien, Daniel A. Dale, Simon C. O. Glover, Ralf S. Klessen, Eric W. Koch, et al.

(2024) ASTRONOMICAL JOURNAL. 167(1).
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Do spiral arms enhance star formation efficiency?

Miguel Querejeta, Adam K. Leroy, Sharon Meidt van der Wel (UGent) , Eva Schinnerer, Francesco Belfiore, Eric Emsellem, Ralf S. Klessen, Jiayi Sun, Mattia Sormani, Ivana Bešlić, et al.

(2024) ASTRONOMY & ASTROPHYSICS. 687.
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Hidden gems on a ring : infant massive clusters and their formation timeline unveiled by ALMA, HST, and JWST in NGC 3351

Jiayi Sun, Hao He, Kyle Batschkun, Rebecca C. Levy, Kimberly Emig, M. Jimena Rodríguez, Hamid Hassani, Adam K. Leroy, Eva Schinnerer, Eve C. Ostriker, et al.

(2024) ASTROPHYSICAL JOURNAL. 967(2).
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JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium

Jérémy Chastenet (UGent) , Ilse De Looze (UGent) , Monica Relaño, Daniel A. Dale, Thomas G. Williams, Simone Bianchi, Emmanuel M. Xilouris, Maarten Baes (UGent) , Alberto D. Bolatto, Martha L. Boyer, et al.

(2024) ASTRONOMY & ASTROPHYSICS. 690.
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PHANGS-JWST : data-processing pipeline and first full public data release

Thomas G. Williams, Janice C. Lee, Kirsten L. Larson, Adam K. Leroy, Karin Sandstrom, Eva Schinnerer, David A. Thilker, Francesco Belfiore, Oleg V. Egorov, Erik Rosolowsky, et al.

(2024) ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 273(1).
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On the Tremaine–Weinberg method : how much can we trust gas tracers to measure pattern speeds?

Olga Borodina, Thomas G. Williams, Mattia C. Sormani, Sharon Meidt van der Wel (UGent) and Eva Schinnerer

(2023) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 524(3). p.3437-3445

Academic Bibliography

Dynamical resonances in PHANGS galaxies

Simulating nearby disc galaxies on the main star formation sequence : I. Bar formation and the building of the central gas reservoir

Neutral atomic and molecular gas dynamics in the nearby spiral galaxies NGC 1512, NGC 4535, and NGC 7496

A 260 pc resolution ALMA map of HCN(1–0) in the galaxy NGC 4321

A two-component probability distribution function describes the mid-IR emission from the disks of star-forming galaxies

Do spiral arms enhance star formation efficiency?

Hidden gems on a ring : infant massive clusters and their formation timeline unveiled by ALMA, HST, and JWST in NGC 3351

JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium

PHANGS-JWST : data-processing pipeline and first full public data release

On the Tremaine–Weinberg method : how much can we trust gas tracers to measure pattern speeds?

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