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Cited article:

Massive Galaxy Mergers Have Distinctive Global H i Profiles

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The Astrophysical Journal 929 (1) 15 (2022)
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SN 2019yvq Does Not Conform to SN Ia Explosion Models

M. A. Tucker, C. Ashall, B. J. Shappee, P. J. Vallely, C. S. Kochanek, M. E. Huber, G. S. Anand, J. V. Keane, E. Y. Hsiao and T. W.-S. Holoien
The Astrophysical Journal 914 (1) 50 (2021)
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On the relationship between gas content, star formation, and global H i asymmetry of galaxies on the star-forming main-sequence

Adam B Watts, Barbara Catinella, Luca Cortese, Chris Power and Sara L Ellison
Monthly Notices of the Royal Astronomical Society 504 (2) 1989 (2021)
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Enhanced atomic gas fractions in recently merged galaxies: quenching is not a result of post-merger gas exhaustion

Sara L Ellison, Barbara Catinella and Luca Cortese
Monthly Notices of the Royal Astronomical Society 478 (3) 3447 (2018)
https://doi.org/10.1093/mnras/sty1247

The frequency and stellar-mass dependence of boxy/peanut-shaped bulges in barred galaxies

Peter Erwin and Victor P. Debattista
Monthly Notices of the Royal Astronomical Society 468 (2) 2058 (2017)
https://doi.org/10.1093/mnras/stx620

IONIZED GAS KINEMATICS AT HIGH RESOLUTION. IV. STAR FORMATION AND A ROTATING CORE IN THE MEDUSA (NGC 4194)

Sara C. Beck, John Lacy, Jean Turner, Thomas Greathouse and Susan Neff
The Astrophysical Journal 787 (1) 85 (2014)
https://doi.org/10.1088/0004-637X/787/1/85

COLD MOLECULAR GAS IN MERGER REMNANTS. I. FORMATION OF MOLECULAR GAS DISKS

Junko Ueda, Daisuke Iono, Min S. Yun, et al.
The Astrophysical Journal Supplement Series 214 (1) 1 (2014)
https://doi.org/10.1088/0067-0049/214/1/1