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1by Santucci, Giulia, Brough, Sarah, van de Sande, Jesse, McDermid, Richard M, van de Ven, Glenn, Zhu, Ling, D'Eugenio, Francesco, Bland-Hawthorn, Joss, Barsanti, Stefania, Bryant, Julia J.“... galaxies. The majority of the galaxies in the sample (73% ± 3%) are oblate, while 19% ± 3% are mildly...”
Published in The Astrophysical Journal
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2by Fogarty, Lisa M R, Scott, N., Owers, M S, Croom, S, Bekki, Kenji, Houghton, Ryan C W, van de Sande, J, D'Eugenio, Francesco, Cecil, Gerald, Colless, Matthew, Bland-Hawthorn, Jonathan, Brough, S, Cortese, L, Davies, Roger L, Sharp, Robert“... with them being oblate spheroids (i.e. discs). The slow rotating ETGs (SRs), on the other hand...”
Published in Monthly Notices of the Royal Astronomical Society
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3by van de Sande, J., Scott, Nicholas, Bland-Hawthorn, J., Brough, Sarah, Bryant, J. J., Colless, Matthew, Cortese, L., Croom, Scott M., D'Eugenio, Francesco, Foster, Caroline, Goodwin, Michael, Konstantopoulos, I. S., Medling, Anne, Sharp, Rob“... observed ellipticity. For the large majority of galaxies that are oblate rotating spheroids, we find...”
Published in Nature Astronomy
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