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The MAGPI Survey: the kinematic morphology-density relation (or lack thereof) and the Hubble sequence at $z\sim0.3$

Fuente: arXiv

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Bibliographic Details
Main Authors:	Foster, Caroline, Donoghoe, Mark W., Battisti, Andrew, D'Eugenio, Francesco, Harborne, Katherine, Venville, Thomas, Lagos, Claudia Del P., Mendel, J. Trevor, Bagge, Ryan, Barsanti, Stefania, Bellstedt, Sabine, Boecker, Alina, Chen, Qianhui, Derkenne, Caro, Ferre-Matteu, Anna, Gjergo, Eda, Gupta, Anshu, Muller, Eric G. M., Santucci, Giulia, Park, Hye-Jin, Remus, Rhea-Silvia, Thater, Sabine, van de Sande, Jesse, Vaughan, Sam, Brough, Sarah, Croom, Scott M., Valenzuela, Lucas M., Wisnioski, Emily, Team, the MAGPI
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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