Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
| Autor: | Rohr, Eric, Pillepich, Annalisa, Nelson, Dylan, Zinger, Elad, Joshi, Gandhali, Ayromlou, Mohommadreza |
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| Rok vydání: | 2023 |
| Předmět: | |
| Zdroj: | MNRAS, 524, 3502-3525 (2023) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1093/mnras/stad2101 |
| Popis: | Jellyfish galaxies are prototypical examples of satellite galaxies undergoing strong ram pressure stripping (RPS). We analyze the evolution of 512 unique, first-infalling jellyfish galaxies from the TNG50 cosmological simulation. These have been visually inspected to be undergoing RPS sometime in the past 5 billion years (since $z=0.5$), have satellite stellar masses $\mstarsat\sim10^{8-10.5}\,M_\odot$, and live in hosts with $\mvir\sim10^{12-14.3}\,M_\odot$ at $z=0$. We quantify the cold gas ($T\leq10^{4.5}$ K) removal using the tracer particles, confirming that for these jellyfish, RPS is the dominant driver of cold gas loss after infall. Half of these jellyfish are completely gas-less by $z=0$, and these galaxies have earlier infall times and smaller satellite-to-host mass ratios than their gaseous counterparts. RPS can act on jellyfish galaxies over long time scales of $\approx1.5-8$ Gyr. Jellyfish in more massive hosts are impacted by RPS for a shorter time span and, at a fixed host mass, jellyfish with less cold gas at infall and lower stellar masses at $z=0$ have shorter RPS time spans. While RPS may act for long periods of time, the peak RPS period -- where at least 50 pecent of the total RPS occurs -- begins within $\approx1$ Gyr of infall and lasts $\lesssim2$ Gyr. During this period, the jellyfish are at host-centric distances $\sim0.2-2\rvir$, illustrating that much of RPS occurs at large distances from the host galaxy. Interestingly, jellyfish continue forming stars until they have lost $\approx98$ percent of their cold gas. For groups and clusters in TNG50 $(\mvirhost\sim10^{13-14.3}\,M_\odot)$, jellyfish galaxies deposit more cold gas ($\sim10^{11-12}\,M_\odot$) into halos than exist in them at $z=0$, demonstrating that jellyfish, and in general satellite galaxies, are a significant source of cold gas accretion. Comment: 20 pages, 11 figures + 3 appendices with 4 figures. Submitted to MNRAS. Key figures are 2, 8, 9, 11. See additional jellyfish companion papers today on astro-ph: Zinger+ and Goeller+. All data used in this publication, including the Cosmological Jellyfish Project results, are publicaly available. Reuploaded after publication |
| Databáze: | arXiv |
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