Physical properties of SDSS satellite galaxies in projected phase space. Issue 2 (14th January 2019)

• Record Type: Journal Article
• Authors: Pasquali, A; Smith, R; Gallazzi, A; De Lucia, G; Zibetti, S; Hirschmann, M; Yi, S K
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 484:Issue 2(2019)
• Page Start: 1702
• Page End: 1723
• Publication Date: 2019-01-14
• Subjects: galaxies: clusters: general -- galaxies: evolution -- galaxies: general -- galaxies: haloes -- galaxies: stellar content; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty3530
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We investigate how environment affects satellite galaxies using their location within the projected phase space of their host haloes from the Wang et al.'s group catalogue. Using the Yonsei Zoom-in Cluster Simulations, we derive zones of constant mean infall time$\overline{T}_{\rm inf}$ in projected phase space, and catalogue in which zone each observed galaxy falls. Within each zone, we compute the mean observed galaxy properties including specific star formation rate, luminosity-weighted age, stellar metallicity, and [α/Fe] abundance ratio. By comparing galaxies in different zones, we inspect how shifting the mean infall time from recent infallers ($\overline{T}_{\rm inf}~\lt$ 3 Gyr) to ancient infallers ($\overline{T}_{\rm {inf}}\gt$ 5 Gyr) impacts galaxy properties at fixed stellar and halo mass. Ancient infallers are more quenched, and the impact of environmental quenching is visible down to low host masses (≤group masses). Meanwhile, the quenching of recent infallers is weakly dependent on host mass, indicating they have yet to respond strongly to their current environment. [α/Fe] and especially metallicity are less dependent on host mass, but show a dependence on$\overline{T}_{\rm {inf}}$ . We discuss these results in the context of longer exposure times for ancient infallers to environmental effects, which grow more efficient in hosts with a deeper potential well and a denser intracluster medium. We also compare our satellites with a control field sample, and find that even the most recent infallers ($\overline{T}_{\rm {inf}}~\lt ~2$ Gyr) are more quenched than field galaxies, in particular for cluster mass hosts. This supports the role of pre-processing and/or faster quenching in satellites.