{ "id": "2402.05788", "version": "v1", "published": "2024-02-08T16:25:20.000Z", "updated": "2024-02-08T16:25:20.000Z", "title": "The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation", "authors": [ "Apashanka Das", "Biswajit Pandey" ], "comment": "19 pages, 10 figures, comments welcome", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We study the evolution of the red and blue galaxies from $z=3$ to $z=0$ using the EAGLE simulation. The galaxies in the blue cloud and the red sequence are separated at each redshift using a scheme based on Otsu's method. Our analysis shows that the two populations have small differences in the local density and the clustering strength until $z=2$, after which the red galaxies preferentially occupy the denser regions and exhibit a significantly stronger clustering than the blue galaxies. The large differences in the cold gas mass and the star formation rate (SFR) of the two populations before $z=2$ indicate that the dichotomy between the two populations may not arise due to the environment alone. The galaxy pairs at each redshift show a significantly higher SFR than the isolated control galaxies within pair separations $<200$ kpc. The SFR of the paired galaxies at a given separation declines with the decreasing redshift, indicating a gradual depletion of their cold gas reservoir. At smaller pair separations, an anomalous increase of the SFR in paired galaxies around $z \\sim 2$, suggests that the environmental effects start to dominate at this redshift, increasing the rate of galaxy interactions and the occurrence of starburst galaxies. We observe a substantial decrease in the blue fraction in paired galaxies starting from $z=1$ to the present. The decrease in the blue fraction is mild for the paired galaxies with their second nearest neighbour at a distance $>500$ kpc.", "revisions": [ { "version": "v1", "updated": "2024-02-08T16:25:20.000Z" } ], "analyses": { "keywords": [ "blue galaxies", "eagle simulation", "paired galaxies", "interactions", "blue fraction" ], "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable" } } }