Ghent University Academic Bibliography

Your filters: cql: author="Barnes, Ashley" or (type any "bookEditor issueEditor" and editor="Barnes, Ashley")

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The gas morphology of nearby star-forming galaxies

Sophia K. Stuber, Eva Schinnerer, Thomas G. Williams, Miguel Querejeta, Sharon Meidt van der Wel (UGent) , Éric Emsellem, Ashley Barnes, Ralf S. Klessen, Adam K. Leroy, Justus Neumann, et al.

(2023) ASTRONOMY & ASTROPHYSICS. 676.
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The impact of H II regions on giant molecular cloud properties in nearby galaxies sampled by PHANGS ALMA and MUSE

Antoine Zakardjian, Jérôme Pety, Cinthya N. Herrera, Annie Hughes, Elias Oakes, Kathryn Kreckel, Chris Faesi, Simon C. O. Glover, Brent Groves, Ralf S. Klessen, et al.

(2023) ASTRONOMY & ASTROPHYSICS. 678.
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PHANGS-JWST first results : a statistical view on bubble evolution in NGC628

Elizabeth J. Watkins, Ashley Barnes, Kiana F. Henny, Hwihyun Kim, Kathryn Kreckel, Sharon Meidt van der Wel (UGent) , Ralf S. Klessen, Simon C. O. Glover, Thomas G. Williams, B. W. Keller, et al.

(2023) ASTROPHYSICAL JOURNAL LETTERS. 944(2).
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The organization of cloud-scale gas density structure : high-resolution CO versus 3.6 μm brightness contrasts in nearby galaxies

Sharon Meidt van der Wel (UGent) , Adam K. Leroy, Miguel Querejeta, Eva Schinnerer, Jiayi Sun, Arjen van der Wel (UGent) , Eric Emsellem, Jonathan Henshaw, Annie Hughes, J. M. Diederik Kruijssen, et al.

(2021) ASTROPHYSICAL JOURNAL. 913(2).
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PHANGS-ALMA data processing and pipeline

Adam K. Leroy, Annie Hughes, Daizhong Liu, Jérôme Pety, Erik Rosolowsky, Toshiki Saito, Eva Schinnerer, Andreas Schruba, Antonio Usero, Christopher M. Faesi, et al.

(2021) ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 255(1).

Academic Bibliography

The gas morphology of nearby star-forming galaxies

The impact of H II regions on giant molecular cloud properties in nearby galaxies sampled by PHANGS ALMA and MUSE

PHANGS-JWST first results : a statistical view on bubble evolution in NGC628

The organization of cloud-scale gas density structure : high-resolution CO versus 3.6 μm brightness contrasts in nearby galaxies

PHANGS-ALMA data processing and pipeline

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