Abstract
Abstract
Here we present a statistical study on tidal features around massive early-type galaxies (ETGs). Utilizing the imaging data of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP), we measure the flux fraction of tidal features (f
tidal) in 2649 ETGs with stellar mass M
* > 1011
M
⊙ and redshift 0.05 < z < 0.15 using automated techniques. The Wide layer of HSC-SSP reaches a depth of ∼28.5 mag arcsec−2 in the i band. Under this surface brightness limit, we find that about 28% of these galaxies harbor prominent tidal features with f
tidal > 1%, among which the number of ETGs decreases exponentially with f
tidal, with a logarithmic slope of ∼100. Within the stellar mass range we probe, we note that f
tidal increases by a factor of 2 from M
* ≈ 1011 to 1012
M
⊙. We also perform a pair count to estimate the merger rate of these massive ETGs. Combining the merger rates with f
tidal, we estimate that the typical lifetime of tidal features is ∼3 Gyr, consistent with previous studies.
Funder
National Natural Science Foundation of China
Chinese Academy of Sciences
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
8 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献