Environmental effects on the UV upturn in local clusters of galaxies




Sadman S. Ali, Malcolm N. Bremer, Steven Phillipps, Roberto De Propris

PublisherOXFORD UNIV PRESS

2019

 Monthly Notices of the Royal Astronomical Society

MON NOT R ASTRON SOC

487

3

3021

3028

8

0035-8711

1365-2966

DOIhttps://doi.org/10.1093/mnras/stz1502

https://academic.oup.com/mnras/article/487/3/3021/5510432

https://research.utu.fi/converis/portal/detail/Publication/42056229



We explore the dependence of ultraviolet (UV) upturn colours in early-type cluster galaxies on the properties of their parent clusters (such as velocity dispersion and X-ray luminosity) and on the positions and kinematics of galaxies within them. We use a sample of 24 nearby clusters with highly complete spectroscopy and optical/infrared data to select a suitable sample of red-sequence galaxies, whose far-ultraviolet and NUV magnitudes we measure from archival GALEX data. Our results show that the UV upturn colour has no dependence on cluster properties and has the same range in all clusters. There is also no dependence on the projected position within clusters or on line-of-sight velocity. Therefore, our conclusion is that the UV upturn phenomenon is an intrinsic feature of cluster early-type galaxies, irrespective of their cluster environment.

Last updated on 26/11/2024 12:49:13 PM