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arXiv · 1805.09341

Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion

Qirong Zhu·Dandan Xu·Massimo Gaspari·Vicente Rodriguez-Gomez·Dylan Nelson·Mark Vogelsberger·Paul Torrey·Annalisa Pillepich·Jolanta Zjupa·Rainer Weinberger·Federico Marinacci·Rüdiger Pakmor·Shy Genel·Yuexing Li·Volker Springel·Lars Hernquist
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Abstract

The galaxy Malin 1 contains the largest stellar disk known but the formation mechanism of this structure has been elusive. In this paper, we report a Malin 1 analogue in the 100 Mpc IllustrisTNG simulation and describe its formation history. At redshift zero, this massive galaxy, having a maximum circular velocity $V_{\rm max}$ of 430 ${\rm km\ s^{-1}}$, contains a 100 kpc gas/stellar disk with morphology similar to Malin 1. The simulated galaxy reproduces well many observed features of Malin 1's vast disk, including its stellar ages, metallicities, and gas rotation curve. We trace the extended disk back in time and find that a large fraction of the cold gas at redshift zero originated from the cooling of hot halo gas, triggered by the merger of a pair of intruding galaxies. Our finding provides a novel way to form large galaxy disks as extreme as Malin 1 within the current galaxy formation framework.

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Qirong Zhu, Dandan Xu, Massimo Gaspari, Vicente Rodriguez-Gomez, Dylan Nelson, Mark Vogelsberger, Paul Torrey, Annalisa Pillepich, Jolanta Zjupa, Rainer Weinberger, Federico Marinacci, Rüdiger Pakmor, Shy Genel, Yuexing Li, Volker Springel, Lars Hernquist. 2018-05-23. Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion. https://doi.org/10.1093/mnrasl/sly111

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